The galaxy presents a generally elliptical morphology with a concentrated central bulge. The light profile appears smooth and relatively featureless, suggesting an older stellar population. There is a discernible color gradient from the core outward, with the central region exhibiting a yellowish hue which transitions to a bluer color in the outer regions. This could imply ongoing star formation in the outskirts. The galaxy seems to be fairly isolated with no obvious signs of tidal interactions or recent mergers, although there is a small disturbance in the bottom of the galaxy, possibly hinting at a previous minor merging event or a small satellite galaxy being consumed. The overall rounded appearance reinforces a classification toward an elliptical or lenticular type galaxy.
