The galaxy appears to be a relatively smooth, elliptical galaxy at a redshift of approximately 0.19, indicating a substantial distance. It exhibits a centrally concentrated luminosity profile, suggesting a dominant bulge component. The galaxy's color appears redder in the central regions, possibly indicative of an older stellar population and a lack of ongoing star formation. A very slight hint of a disk may be present, with a more diffuse and bluer stellar population surrounding the red core. There are no prominent spiral arms or dust lanes visible. The galaxy appears somewhat elongated in shape, and no significant signs of interaction or major disturbances are immediately apparent, although there is a potential minor disturbance. The estimated size is approximately 7.6 kpc in radius. The galaxy's mass is estimated to be around 10^10.9 solar masses. The star formation rate is estimated to be about 10^-1.5 solar masses per year, which is relatively low. The specific star formation rate is estimated to be around 10^-12.5 per year, indicating that the galaxy is not actively forming many new stars.
