The galaxy presents a primarily smooth morphology. Its overall shape appears roughly circular, with a slight deviation towards an elliptical form. There is evidence of a possible merger event. A minor disturbance is visible within the galaxy's structure, hinting at interactions with another galaxy or tidal forces, suggesting a system undergoing dynamical change. Although a central bulge is not immediately apparent, the galaxy's relative uniformity points to a relatively old stellar population dominating its composition, with a significant portion of the stellar mass concentrated in the spheroid. The galaxy exhibits a redder color, suggestive of a population of older stars with lower metallicity. This galaxy shows some signs of disturbance which might be related to the ongoing process of galaxy evolution, especially in terms of its shape and internal structure.
