The galaxy presents as a generally smooth object with a slightly elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant bulge component. There is a subtle color gradient observed, with the core appearing more yellowish-white and the outer regions having a slightly bluer tint. There is no strong evidence of prominent spiral arm structures or significant dust lanes. The galaxy does not appear to be undergoing any major merger events, although there are some indications of minor asymmetry or disturbance in the outer halo.
