The galaxy presents a relatively smooth, elliptical morphology. There is a distinct central bulge region that appears bright and concentrated, gradually fading outwards to a more diffuse halo. The light distribution suggests a well-mixed stellar population with a dominant older component, evident from the yellowish to reddish hue concentrated in the core. There is little indication of significant dust lanes or prominent spiral arm structures. Based on visual inspection, the galaxy does not show evidence of major mergers or tidal disturbances, appearing relatively isolated and undisturbed. The shape is closer to round than cigar-shaped, tending towards being an elliptical galaxy. Overall, it displays characteristics consistent with an early-type galaxy that is not currently experiencing a high rate of star formation.
