The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, largely featureless morphology. The light distribution is centrally concentrated, with a moderate ellipticity, appearing more rounded than elongated. The color index suggests a relatively evolved stellar population, leaning towards redder hues across the observed spectrum. There is no apparent evidence of spiral arms, prominent dust lanes, or ongoing major mergers. Minor tidal disturbances or faint, unresolved features cannot be entirely ruled out at this resolution. The overall appearance indicates a system dominated by older stars, with limited recent or ongoing star formation.
