This galaxy exhibits a mostly smooth morphology, with a notable absence of distinct spiral arm structures or prominent dust lanes. The light distribution appears relatively uniform, indicative of an elliptical or lenticular galaxy type. Its overall color profile suggests an older stellar population. There is evidence of a possible minor disturbance on the left of the main galaxy, with an apparent secondary object or region of altered light distribution. The main body of the galaxy shows a round or nearly round shape, without significant elongation or asymmetry. While appearing mostly isolated, the slight irregularity implies a past or ongoing interaction, but it does not present as a currently merging system based on these characteristics.