The galaxy presents as a moderately luminous object with an overall elliptical morphology. Its color profile indicates a predominantly older stellar population, evidenced by its reddish-yellow hue, particularly concentrated in the central bulge. There is a suggestion of a disk-like component, although it is not sharply defined, and appears relatively smooth with limited discernible structure, such as distinct spiral arms or prominent star-forming regions. Some asymmetry is present, with a slight elongation suggesting a possible interaction or disturbance. The galaxy does not appear to be undergoing a major merging event, though there may be some signs of minor tidal disturbance in its outer regions.
