The galaxy appears to be a relatively smooth, elliptical-type galaxy, with a noticeable central bulge. It exhibits a slightly elongated shape, appearing somewhere between round and cigar-shaped. The color gradient suggests an older stellar population, with a yellowish hue dominating the galaxy's light. There is a faint, diffuse halo surrounding the central region, with no apparent spiral arms or distinct dust lanes. Based on the light distribution, the majority of the galaxy's mass seems concentrated towards the center. There is a possibility of a minor tidal disturbance, though the smoothness suggests that it is likely in its late stages. The galaxy does not appear to be undergoing a major merger.
