The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A significant bulge component is apparent, dominating the overall light distribution. The galaxy exhibits a color gradient, appearing more reddish-yellow towards the core and transitioning to a slightly bluer hue in the outer regions. This color variation could indicate differing stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars populating the outer disk. There is no clear evidence of prominent spiral arms or a distinct disk structure, rather it seems to be a spheroid shape. There appear to be signs of minor disturbances, however it is not thought to be undergoing a merging event. It appears to be moderately massive and is undergoing some star formation.
