The galaxy appears as an elliptical-type galaxy, exhibiting a smooth, concentrated morphology without prominent spiral arms or a distinct disk structure. The light distribution suggests a largely homogenous stellar population. There is a slight elongation in shape, deviating marginally from a perfectly circular form. The galaxy's color index suggests an older stellar population, potentially indicating a lack of significant ongoing star formation activity. The overall structure displays no evidence of major mergers or tidal disturbances. There is, however, a possible minor disturbance in the halo region, such as a dust cloud or tidal stream. The galaxy displays redder colors, potentially correlating to the presence of an older stellar population and minimal active star formation.
