The galaxy appears as a centrally concentrated object with a relatively smooth morphology. There is a slight elongation, but the overall shape is generally round. The color profile indicates the presence of an older stellar population, with a reddish hue dominating the light output. There is very little indication of spiral arm structure, or prominent dust lanes. The galaxy does not appear to be undergoing any major merging activity. Based on its red color, and lack of distinctive features, it may be classified as an elliptical galaxy.
