The galaxy presents as an elongated, cigar-shaped object, with a generally smooth appearance. There is a concentration of light toward the center of the galaxy, indicating a possible bulge. The color profile suggests a redder core transitioning to slightly bluer hues in the outer regions, which could indicate older stellar populations concentrated in the center and younger, star-forming regions in the disk. There are hints of some disturbed features, potentially minor tidal interactions or internal dynamics causing asymmetry. However, on the whole it appears mostly undisturbed. The overall structure points towards an elliptical galaxy, possibly with a disk-like component.
