The galaxy presents as a relatively smooth, elliptical morphology. The overall color appears to be a yellowish-red hue, potentially indicating an older stellar population with diminished recent star formation. There is a high degree of central concentration, with light intensity decreasing gradually towards the outer edges of the galaxy. There is no clear evidence of spiral arms or a prominent disk structure. Slight asymmetry may be present in the outer regions, though it is difficult to say definitively due to the image resolution. There are no obvious signs of recent merger activity or major tidal disturbances.
