The galaxy appears to be an elliptical galaxy, characterized by a largely featureless and smooth morphology. The light distribution seems concentrated towards the center, with a gradual decline in brightness outwards. The central region exhibits a relatively high surface brightness. There is a slight elongation of the galaxy along one axis, giving it an intermediate shape between round and cigar-shaped. No distinct spiral arms or bar structures are discernible. Based on the color information, the galaxy appears to be dominated by older stellar populations, emitting primarily in the redder wavelengths, with a possible contribution from younger, bluer stars in the central region, although the overall color suggests a low rate of on-going star formation. There's no obvious sign of recent major merger activity, such as tidal tails or strong morphological disturbances, although minor interaction cannot be fully excluded.
