This galaxy exhibits a relatively smooth morphology, with a notable absence of distinct spiral arms or a well-defined disk structure. It appears elliptical in shape, displaying an intermediate axis ratio, neither perfectly round nor highly elongated. A central bulge is evident, characterized by a bright, concentrated core. The color profile suggests the presence of a relatively older stellar population, exhibiting bluer hues. There is no indication of ongoing major merger activity, however there is a small chance that the galaxy is currently undergoing minor interactions or experiencing some internal disturbances, though these are not immediately apparent.
