The galaxy presents a generally smooth appearance, with a high concentration of light toward the center, suggesting a prominent bulge. The shape appears somewhat elongated or cigar-shaped, deviating from a perfectly circular disk or spheroid. While the overall structure seems relatively undisturbed, there are subtle hints of asymmetry or minor perturbations in the outer regions of the galaxy, but no obvious signs of major merging activity. The color profile indicates the presence of both older stellar populations dominating the central regions, exhibiting a yellowish-orange hue, and slightly bluer regions toward the outer edges, potentially indicating ongoing star formation activity.
