The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated, luminous core region exhibiting a yellowish hue.  The light intensity decreases gradually from the core outwards, transitioning to a bluer halo.  The galaxy appears to be more elongated than circular, with a cigar-like morphology. There is no obvious indication of spiral arm structure or significant dust lane features.  There appears to be a low chance of disturbances due to merging.
