The galaxy presents as a primarily smooth, elliptical-like structure, though not perfectly spherical. It displays a concentrated central bulge region that is bright and appears more luminous than the surrounding areas of the galactic disk. The galaxy is elongated, appearing cigar-shaped, but the primary visible component appears largely undisturbed, with no obvious signs of major mergers. The outer regions exhibit a faint, diffuse glow, indicating the presence of a stellar halo. There is a suggestion of subtle structural features, but due to image resolution, it is challenging to definitively identify the presence of spiral arms or other disk structures. Color gradients suggest a potentially older stellar population dominating the bulge, with bluer hues in the outer regions that imply more recent star formation activity. There is a subtle asymmetry to the galaxy's profile, potentially indicating a minor interaction or internal dynamic.
