The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution across its structure. There appears to be minimal evidence of spiral arms or significant dust lanes. The galaxy displays a dominant central bulge with a concentrated region of high luminosity. A slight elongation is noticeable, classifying it as more 'in between' oval shaped. The color profile suggests a predominantly older stellar population. There is no clear sign of ongoing major mergers, but there is a potential indication of a slight disturbance in the outer regions of the galaxy which could suggest a minor past merging event. Star formation is low.
