The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A prominent bulge region is observed, exhibiting a reddish hue suggestive of an older stellar population. The outer regions display a fainter, more diffuse halo with a bluer color, potentially indicative of ongoing or recent star formation. The galaxy's shape deviates noticeably from a perfect circle, with a discernible elongation, suggesting a possible cigar shape. No obvious spiral arm structures or significant dust lanes are apparent within the resolution of this image, and no obvious evidence of a major merger or tidal disturbance is observed.
