The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a bright, concentrated luminosity, suggesting a high stellar density or potentially an active galactic nucleus. The overall color profile indicates a population dominated by older stars, with a subtle reddening toward the central bulge. The galaxy appears largely undisturbed, lacking prominent spiral arms or significant tidal features, with an estimated physical size that is fairly compact. The slight elongation in its shape suggests an elliptical morphology somewhere between perfectly circular and more cigar-shaped. Faint, indistinct features might be present in the outer regions, but the resolution limits definitive characterization. The rate of star formation is inferred to be very low.
