The galaxy presents as a single, concentrated object with a smooth and largely featureless morphology. It exhibits a generally elliptical shape, appearing almost perfectly round. The color profile appears to be dominated by light at the redder end of the spectrum, indicating a population of older stars and minimal ongoing star formation. The galaxy's core displays a significantly higher surface brightness than its outer regions, suggesting a dense stellar population concentrated towards the center. There is no visible evidence of spiral arms, bar structures, or significant dust lanes. The overall impression is that of a well-formed, relatively evolved elliptical galaxy. There is no significant evidence of any merging activity.