The galaxy appears to be an elliptical type, characterized by a smooth, largely featureless morphology. Its overall shape is generally round. There is a concentration of light in the center, suggesting a bulge. The galaxy exhibits a subtle color gradient, with the central region appearing somewhat redder than the outer parts, which are slightly bluer. This may indicate an older stellar population in the core, and ongoing or recent star formation in the galaxy's outer regions. The light is evenly distributed, lacking any noticeable spiral arms, bars, or dust lanes. There is no evidence of any major ongoing merging activity or significant tidal disturbances.
