The galaxy presents as a centrally concentrated, relatively smooth object. A discernible disk is present, but does not dominate the morphology. The central bulge exhibits a bright, concentrated luminosity profile, indicative of a high stellar density. The overall shape appears moderately elliptical, leaning slightly towards a rounder, but not perfectly spherical, form. Subtle asymmetries are observed in the outer regions, suggesting possible minor gravitational disturbances or past interactions. There may be weak evidence of recent or ongoing star formation within the disk component, possibly slightly less than would be expected based on its mass. The colors suggest a population of intermediate to old stars, with the central region slightly redder in color, while the surrounding disk appears slightly bluer. There is no obvious signature of a major merger event; however, subtle features may suggest a minor disturbance or interaction.
