The galaxy presents as an elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the light gradually diminishes. There appears to be a relatively smooth transition from the bulge to the outer regions. There is a slight flattening visible, with the galaxy being more elongated than spherical. The lack of distinct spiral arms or prominent dust lanes supports its classification as an elliptical galaxy. The overall color is indicative of a mature system, implying a low rate of current star formation. There may be some ongoing, low-level star formation in the outer regions, hinted at by a slight bluer color, but it is not significant. There are no obvious signs of a major ongoing merger or strong tidal distortions. Overall, it appears to be an isolated and relaxed elliptical galaxy.
