The galaxy presents as a largely smooth, elliptical morphology. It appears to be a relatively mature system, with a dominant spheroidal component. The central bulge is bright and concentrated, exhibiting a yellowish-red hue, indicative of an older stellar population. Fainter and bluer components are visible at the edges of the disk. There are no obvious spiral arm structures visible, suggesting the galaxy is likely not actively forming many new stars. Overall, the galaxy displays a relaxed, symmetrical appearance, though there is the slightest asymmetry to the upper right edge. There is no evidence of major mergers or significant tidal disturbances in its immediate environment, although there could be some minor activity.
