The galaxy presents an overall smooth, elliptical morphology. There is a slight elongation, but it primarily appears to be spheroidal. The color profile suggests a population of older stars, with a redder hue dominating. However, there are also subtle variations in color, including some regions exhibiting bluer tints that possibly suggest areas of more recent, though subdued, star formation. No distinct spiral arms, bars, or other significant structural features such as tidal tails or obvious dust lanes are discernible. There is a very slight asymmetry which could point to a very minor merger event in the recent past. The galaxy lacks a bright, concentrated nucleus; instead, the light is diffusely distributed. The absence of prominent features indicates a relatively quiescent galaxy.
