The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity outwards. The core region appears yellowish-white, suggesting an older stellar population. There's minimal evidence of spiral arm structure or significant dust lanes. Based on the apparent roundness, the galaxy is observed at a small inclination angle relative to our line of sight. There are no obvious signs of recent or ongoing major merger activity, though there may be subtle indications of minor disturbances in the outer regions. The galaxy seems to be relatively isolated, with no immediate, obvious companion galaxies disrupting its structure.
