The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a centrally concentrated luminosity profile with a gradual decline in intensity towards the outer regions. There is no clear evidence of spiral arms or a distinct disk. The galaxy appears somewhat rounded, with only a very slight elongation. There is no obvious sign of any current major merging activity or strong tidal disturbances, although there are faint hints of minor asymmetry. The galaxy displays a general yellowish-white hue, suggesting a relatively older stellar population, and reduced ongoing star formation.
