The galaxy appears to be a relatively compact object, exhibiting a primarily smooth morphology. It displays a generally elliptical shape. There is a distinct color gradient, with the central region showing a yellow-orange hue, suggesting an older stellar population. Fainter, diffuse regions are seen extending outwards. Patches of bluer light are also observed, indicating regions of younger, hotter stars, possibly due to ongoing star formation activity, albeit at a low rate. There is no clear evidence of spiral arms or a prominent disk structure. There is no presence of a major ongoing merger. Overall, the galaxy appears to be a moderate-sized system.
