The galaxy presents as a moderately luminous, relatively compact system. Its morphology appears generally elliptical, exhibiting a smooth, centrally concentrated luminosity profile. The light distribution is not perfectly circular but displays a slight elongation along one axis, tending towards a more oblate shape.

The galaxy’s color profile exhibits a central region with a distinctly redder hue, transitioning to a bluer tint in the outer regions. This suggests a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outskirts. 

There is no evidence of spiral arms or a bar structure. Minor asymmetries may be present, potentially indicative of past minor merger events or internal disturbances, but this galaxy appears as a largely undisturbed system.
