The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. It presents an overall yellowish hue in the central region, with a gradual color gradient toward the outer edges, shifting towards redder tones. The shape is somewhat elongated, but predominantly smooth, indicating a low level of active star formation, in conjunction with a likely older stellar population within its core. There is little evidence of spiral arms or significant dust lanes. The outer halo appears diffuse, blending seamlessly into the background sky, suggesting a lack of sharp boundaries. A slight asymmetry in the distribution of light may suggest a minor gravitational interaction or past merger event, although no clear tidal tails or other major disturbances are evident.