The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology with a high degree of central concentration. It exhibits a cigar-like shape, suggesting it is an elongated ellipsoid. There is a color gradient visible, with a yellowish or golden hue concentrated towards the core, indicative of an older stellar population and lower levels of ongoing star formation. The outer regions show a bluer tint, which could indicate the presence of some younger stars or a population with lower metallicity. The galaxy lacks any distinct spiral arms or bar structures. There is no significant evidence of tidal disturbances or merging activity in this image, though subtle perturbations cannot be ruled out.
