The galaxy presents as a single, relatively smooth object with a centrally concentrated brightness profile. There is little evidence of spiral arm structures or prominent dust lanes. The galaxy exhibits a roughly elliptical morphology, appearing mostly round, with a subtle elongation. The color gradient suggests a somewhat older stellar population, with a yellowish hue in the core transitioning to slightly bluer tones in the outer regions. There are no apparent signs of a major ongoing merger or significant tidal disturbances.
