The galaxy exhibits a generally smooth morphology with a slight elongation in shape. The light distribution appears concentrated towards the center, suggesting the presence of a prominent bulge. The color profile indicates a relatively old stellar population, as evidenced by the redder hues concentrated in the central regions. There are faint indications of a possible disk component, but no distinct spiral arms or bar structures are discernible. Minor disturbances in the outer regions may suggest past or ongoing interactions, however, the galaxy displays a structure generally consistent with a non-merging system. The color suggests relatively low levels of on-going star formation. The galaxy appears to be a lenticular or early-type spiral galaxy, dominated by older stars and a substantial bulge.
