The galaxy presents a predominantly smooth morphology, lacking any prominent spiral arms or distinct features associated with active star formation regions. Its shape appears largely rounded, with only minor deviations from a perfectly circular profile. There is no indication of a recent or ongoing major merger event disrupting the galaxy's structure, although subtle signs suggest a possible minor disturbance. The central region exhibits a concentrated luminosity, indicative of a significant stellar population, likely composed of older stars. Overall, the galaxy's appearance aligns with that of an elliptical galaxy, characterized by a spheroid-like structure and a generally quiescent star formation rate.
