The galaxy presents as a single, centrally concentrated object with a generally smooth morphology. The light profile appears centrally bright, gradually diminishing outwards. Coloration exhibits a central yellow-orange hue, indicative of an older stellar population dominating the core region. The outer regions display a slightly bluer tint, suggesting the presence of younger stars, although the overall star formation rate appears low. The overall shape is close to circular, showing minimal signs of significant disturbances or tidal features. There may be a faint disk like structure, but it is difficult to tell. No distinct spiral arms or bar structures are readily apparent. There are no other galaxies or objects in the FOV to suggest a recent merging event.
