The galaxy appears as an elliptical structure with a bright, concentrated central bulge that exhibits a yellowish hue, suggestive of an older stellar population. The galaxy's outer regions display a bluer tint, indicating the presence of younger stars and possible ongoing star formation, albeit at a moderate level. The overall shape is elongated, but not exceptionally so, appearing somewhat in between circular and cigar-shaped. There is no strong evidence of spiral arms or significant disk features. No major mergers or significant tidal disturbances are apparent in the image, although subtle irregularities in the outer envelope cannot be ruled out at this resolution.
