The galaxy presents as a moderately bright, centrally concentrated object. Its overall form appears relatively smooth, with a slightly elliptical morphology. There are no prominent spiral arms or bar structures visible in this image. The galaxy exhibits a gradual decrease in surface brightness from the core outwards, suggesting a lack of significant ongoing star formation within the central regions. There is a small amount of possible disk, although this is not certain. There are no obvious signs of a major merger event or significant tidal disturbances, but there may be a small amount of ongoing disturbance. The color profile suggests a redder stellar population, typical of an evolved galaxy with a diminished star formation rate. The galaxy's estimated size appears substantial, possibly indicating a relatively massive system.
