The galaxy presents as a relatively smooth and concentrated object. Its overall morphology appears elliptical, lacking any distinct spiral arm structures. The central region exhibits a brighter, more intense luminosity, suggesting a dense stellar population or an active galactic nucleus. The outer regions gradually fade in intensity, indicating a decreasing density of stars and interstellar matter with increasing radial distance from the core. The color profile suggests a population dominated by older stars, as indicated by the reddish-yellow hue, with limited evidence of ongoing, significant star formation. Minor distortions in the overall shape are observable, which could suggest a merger with a smaller galaxy. 
