The galaxy presents as a smooth, elliptical-like structure, with a concentrated central bulge. The color gradient transitions from a yellowish core to a redder periphery, suggesting an older stellar population dominating the central region, potentially with less dust obscuration. The outer regions are less defined, fading gradually into the background, hinting at a lack of prominent spiral arms or strong star-forming regions. The axial ratio suggests the galaxy is somewhat elongated, appearing cigar-shaped rather than perfectly circular. There is no visible evidence of major mergers or strong tidal disturbances; the galaxy appears relatively isolated and undisturbed. The overall morphology indicates a relatively passive, evolved system, with little ongoing star formation.
