The galaxy appears to be a relatively compact object, exhibiting a generally smooth morphology. It presents as an elliptical or lenticular galaxy, with a subtle elongation suggesting a flattened spheroidal shape, but no readily apparent spiral arm structure. The light distribution is centrally concentrated, with a diffuse, fainter halo extending outwards.

The color gradient shows a slightly bluer core, transitioning to redder hues in the outer regions. This color variation may indicate ongoing or recent star formation in the central regions, possibly with an aging stellar population dominating the outer parts. There is no evidence of strong dust lanes or significant tidal distortions, suggesting a relatively settled state. Minor disturbances may be occurring, however there is nothing significant that can be noted. The galaxy is also exhibiting relatively low levels of star formation.
