The galaxy presents as a somewhat elongated structure, appearing cigar-shaped. It exhibits a concentrated central bulge with a noticeable radial gradient in luminosity, fading outwards. There is a suggestion of a disk component, though it appears disturbed or irregular. The overall color is relatively red, indicating a population of older stars and/or significant dust obscuration. There isn't strong evidence of distinct spiral arms, but subtle asymmetries suggest potential minor gravitational interactions or past merger events, though the majority of light appears to be undisturbed. The galaxy appears relatively smooth in its overall light distribution.
