The galaxy presents an elliptical morphology, appearing largely smooth in structure. Its color profile is centrally concentrated, exhibiting a yellowish-white hue that gradually fades towards its outer regions. The galaxy shows a slight elongation, appearing more cigar-shaped than perfectly round. There is no indication of prominent spiral arms or significant dust lanes. The overall appearance suggests a relatively evolved system with a likely high degree of stellar population homogeneity. There is no visible evidence of ongoing major mergers or significant tidal disturbances, the system appears largely undisturbed. The light distribution indicates a concentrated central bulge, further supporting the elliptical classification.
