This galaxy presents as an elliptical morphology, with a smooth light distribution characteristic of an early-type galaxy. The central region exhibits a pronounced red hue, suggesting an older stellar population and a lack of ongoing star formation within the nucleus. Moving outwards from the core, the color transitions towards a more yellowish-white, potentially indicating the presence of a somewhat younger stellar population or a difference in metallicity gradients.

The overall shape is moderately elongated, displaying a deviation from perfect circularity. There is evidence of faint tidal features, potentially indicating a past or ongoing interaction with a smaller companion galaxy or a more distant neighbor. These faint disturbances suggest a level of recent activity that may influence the galaxy's morphological evolution. Based on the colors, the galaxy appears to be at an intermediate distance, exhibiting characteristics of a massive system with a relatively low star formation rate.
