The galaxy appears as a somewhat elliptical or lenticular system. The central bulge exhibits a bright, concentrated luminosity with a yellowish hue, suggesting a population of older stars. Moving outward from the core, a fainter, bluer disk is observed, though it lacks distinct spiral arm structures. There is a subtle flattening of the galactic shape, but overall the system presents with relatively smooth features. Some minor asymmetry or disturbance seems to be present. The galaxy does not appear to be undergoing a major merger or significant interaction with other galaxies. There are no prominent dust lanes visible. Star formation is likely occurring at a very low rate.
