The galaxy presents as a cigar-shaped morphology, exhibiting an elongated, elliptical structure. The light distribution appears relatively smooth, suggesting a dominant spheroid component. A subtle color gradient is observed, with a slight concentration of greenish hues toward the central regions, possibly indicating the presence of younger stellar populations or ionized gas. The outer regions transition to a more reddish-yellow hue, which could suggest older, redder stellar populations dominating at larger radii. There is no obvious indication of a strong spiral arm structure, prominent dust lanes, or ongoing major mergers. Faint asymmetric structures are hinted at, potentially minor tidal disturbances or faint outflows.
