The galaxy presents as a generally elliptical morphology with a smooth, concentrated light distribution. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively isolated, showing no signs of ongoing major mergers or tidal interactions. The color profile suggests a population dominated by older stars, with a gradual shift toward slightly bluer hues in the outskirts, potentially indicating some ongoing or recent star formation in the outer regions. The galaxy's core appears well-defined and centrally located within the overall structure. Given the observed characteristics, this object can likely be characterized as an early-type galaxy, possibly an elliptical galaxy or a lenticular galaxy viewed at a large inclination angle.
