The galaxy presents as a relatively smooth and luminous object, concentrated towards a bright central core. The morphology appears to be largely spheroidal. There is a distinct lack of discernible spiral arm structure or prominent dust lanes. The galaxy exhibits a color gradient, with the core appearing more yellow-white, and the outer regions having a reddish hue. This suggests an older stellar population dominating the core, and a presence of either redder stars or dust in the outskirts. The galaxy does not appear to be actively merging or undergoing any significant tidal disruption, and has a very small percentage of disturbances based on the smooth or featured classification. The galaxy appears well defined and not particularly elongated.
