The galaxy presents a largely smooth morphology, appearing somewhat elliptical in shape. The central region exhibits a concentrated, bright core, indicative of a substantial stellar population or potentially an active galactic nucleus. Moving outwards from the core, the galaxy displays a gradual decrease in luminosity, transitioning into a less defined outer halo. There is a subtle color gradient evident, with the core exhibiting a yellowish hue, suggestive of older stellar populations, while the outer regions show hints of bluer tones, possibly indicating the presence of younger stars or ongoing star formation. No distinct spiral arms or bar structures are readily apparent, which supports its classification as a relatively undisturbed elliptical galaxy. Faint irregular features, such as minor disturbances or tidal tails, are not clearly visible, suggesting the absence of recent major merger events. Overall, the galaxy appears to be a relatively quiescent system, dominated by older stellar populations and a smooth, featureless structure.
