The galaxy presents as a generally smooth, elliptical form. The light distribution is centrally concentrated with a gradual decline in surface brightness moving outwards. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. A surrounding halo appears bluish, potentially suggesting the presence of younger, hotter stars contributing to star formation activity. The galaxy lacks a clear disk structure or spiral arms. There may be a very slight irregularity in the outer regions, possibly indicating a minor tidal interaction or internal disturbance, but the dominant impression is one of relative symmetry and quiescence.
