The galaxy presents as a somewhat elliptical structure, with a smooth, concentrated central bulge that exhibits a yellowish-white hue, potentially indicating an older stellar population. The disk appears relatively smooth and lacking in distinct spiral arm structures. The overall color profile appears to be trending towards the redder end, which could suggest a lower rate of ongoing star formation relative to other galaxies. There may be faint dust lanes or irregularities visible within the disk, but these features are subtle. The galaxy lacks any sign of active galactic nuclei or any recent merger activity. The light distribution, with the central bulge brightness rapidly decreasing towards the edge, suggests a Sersic profile.
