The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. It presents a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The overall shape is somewhat elongated, showing a departure from perfect sphericity, but not dramatically so. The color profile suggests an older stellar population, indicated by the redder hue in the central regions, shifting slightly towards bluer tones in the outer regions, suggesting a low level of ongoing star formation. There is no apparent disk or spiral structure visible within the limits of the data quality. There are no signs of any merger activity or significant tidal disturbances in its immediate environment.
