The galaxy presents as an elliptical morphology, exhibiting a largely smooth and centrally concentrated light distribution. The core region displays a yellowish hue, potentially indicative of an older stellar population dominating the central region. Moving outwards, the color transitions to a bluer tone, suggesting the presence of younger, hotter stars in the outer regions.

There is no discernable disk structure, spiral arms, or bar. The galaxy appears to be relatively undisturbed, showing no signs of major merging events or significant tidal interactions. A slight asymmetry may be present in the outer regions of the galaxy, but it does not appear to be highly irregular. The size of the galaxy is relatively compact, with a moderately high luminosity given its inferred distance. Star formation appears to be present, but not at extremely high levels. 
