The galaxy presents as a generally smooth and centrally concentrated object, with a slight elongation. The core region exhibits a bright, compact morphology, indicative of a high stellar density or the presence of an active galactic nucleus. Fainter, diffuse light extends outward from the core, fading into the background. The overall color appears somewhat blueish, suggesting the presence of some young, hot stars contributing to the overall luminosity. There is no clear evidence of spiral arms or a distinct disk structure in this image, possibly indicating that it is an elliptical or lenticular galaxy. There also does not appear to be a major merger happening. There appears to be a slight disturbance occurring in the distribution of the galaxy's light and possibly some mild tidal features, indicative of past interactions or accretion events.
