The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits a morphology consistent with an early-type galaxy, specifically exhibiting characteristics of an elliptical galaxy, but it is not perfectly round. A slight deviation from perfect circularity suggests it leans toward an oblate spheroid shape. There appears to be little to no evidence of distinct spiral arms or a prominent disk structure. The galaxy's light profile is relatively homogenous and appears to lack significant dust lanes or prominent star-forming regions. While the majority of the light is centrally concentrated, there is some presence of diffuse light extending outwards from the core. Overall, it appears as a relatively undisturbed, evolved galaxy. The color index suggests a population dominated by older stars, with a redder hue indicative of low levels of recent star formation. A very minor perturbation or possible faint tidal feature could be present, but the galaxy is largely isolated.
