The galaxy presents as a relatively smooth, elliptical-like structure. The core region displays a concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. There is a slight blue tint towards the outer regions of the galaxy, suggesting the presence of younger, hotter stars, while the central region appears more yellow, potentially indicating an older stellar population. There is no obvious evidence of strong spiral arms or significant dust lanes. The galaxy appears to be fairly isolated with no obvious signs of recent or ongoing major merging activity, although a minor disturbance cannot be completely ruled out. The overall morphology leans towards a round shape.
