The galaxy presents an elliptical morphology, elongated along a discernible axis. Its light distribution is centrally concentrated, exhibiting a smooth, featureless profile without prominent spiral arms or distinct substructures. The core region displays a bright, diffuse glow, suggestive of a high stellar density. Moving outwards from the core, the light gradually diminishes into a fainter halo, implying a decrease in stellar population density. The color gradient suggests an older stellar population, more prominent at the core, with a subtle shift towards slightly bluer tones in the outer regions, which could indicate regions of modest recent star formation. There is no clear indication of ongoing major mergers or significant tidal disturbances in this image. Overall, this galaxy appears to be a relatively undisturbed, early-type system.
