The galaxy presents as a relatively smooth, well-defined elliptical structure. It exhibits a concentrated central bulge of luminous material, likely composed of older stellar populations. Moving outward from the core, the light distribution gradually decreases. I observe minimal evidence of spiral arms or active star formation regions within the galaxy's disk, which is consistent with a low specific star formation rate. The overall color indices suggest a relatively evolved galaxy, potentially indicating a large fraction of old stars and low dust content. Based on the apparent smoothness and shape, this object may be classified as an elliptical galaxy with a high degree of rotational symmetry. There is no evidence of ongoing major mergers or significant tidal disturbances in this galaxy.
