The galaxy presents as a generally smooth, centrally concentrated object. Its overall shape is elliptical, appearing moderately elongated, falling between round and cigar-shaped. A distinct central bulge is visible, with the luminosity gradually decreasing towards the outer regions. There is a subtle color gradient observed, with a slightly yellower or redder hue dominating the central bulge compared to the bluer, fainter regions in the outer disk. No prominent spiral arm structures or significant dust lanes are apparent in this image, suggesting a lack of active star formation regions. There appears to be no indication of ongoing major merger activity or significant tidal disturbances affecting its morphology.
