The galaxy presents as a relatively compact, smooth, and elliptical-like structure with a slight elongation. There is no clear spiral arm structure evident, suggesting a classification tending toward early-type. The color profile of the galaxy suggests the presence of an older stellar population, given its redder hue. Minimal dust lanes or active star-forming regions are discernible, implying a relatively low star formation rate. There are no signs of tidal tails or other indications of recent major merger events, though minor disturbances cannot be ruled out. Overall, the galaxy appears well-defined and quiescent, indicating a stable and evolved system.