The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. It exhibits a bright, unresolved core region, possibly indicative of an active galactic nucleus or a dense stellar population. Extending outwards from the core is a more diffuse, lower surface brightness halo or disk component. The colors appear bluer towards the central region, suggesting the presence of younger, hotter stars, or potentially higher rates of star formation. The outer regions appear redder, indicating older stellar populations. There are no prominent spiral arms, bars, or other distinct features visible within the galaxy's structure, but there may be very faint hints of disturbances in the outer disk, such as asymmetries or tidal features, though these are very subtle. Overall, the galaxy appears to be a relatively undisturbed system, without obvious signs of ongoing major mergers or interactions.
