The galaxy presents a roughly elliptical morphology, appearing somewhat smooth in overall structure. A central bulge region is evident, exhibiting a higher concentration of luminosity. The light distribution suggests a relatively evolved system with a primarily older stellar population. Some faint indications of a disk structure may be present but are not well defined. There may be minor disturbances in the structure, potentially indicative of past or ongoing interactions. Overall, this galaxy appears to be relatively massive with indications of low ongoing star formation.
