The galaxy presents a largely smooth morphology, suggesting a classification leaning toward elliptical or lenticular types. The light distribution appears centrally concentrated with a bright core, indicative of a possible bulge. The galaxy exhibits a slightly elongated shape, appearing more "in between" round and cigar-shaped. There is a subtle suggestion of a disk-like component, but no distinct spiral arms are visible in this image. Overall, the galaxy seems relatively undisturbed, with only minor indications of any significant merger activity. The color profile suggests moderate star formation activity. The galaxy appears to be of intermediate mass.
