The galaxy appears as a moderately bright, centrally concentrated object with a generally elliptical morphology. The light distribution seems smooth, lacking strong spiral arm features or prominent dust lanes. There is a suggestion of a slight elongation, but the overall appearance is close to circular. The color profile indicates a relatively older stellar population, with the galaxy exhibiting a redder hue centrally, fading to a bluer hue near the edges of the galaxy. There is little to no evidence of ongoing major merging activity or significant tidal disturbances based on its morphology. The galaxy displays properties consistent with a relatively quiescent system.