The galaxy presents as a smooth, centrally concentrated object with an ellipsoidal morphology. The light distribution appears relatively even, exhibiting a gradual decline in brightness from the core outward, suggestive of an early-type galaxy or a late-type galaxy viewed edge on. There is a subtle color gradient observed, transitioning from a bluer core to slightly redder outer regions. The overall structure appears largely undisturbed, with no obvious signs of significant tidal interactions or major mergers. Subtle irregularities in the outer isophotes may indicate minor disturbances or past interactions. There appears to be a degree of star formation activity in the central region.
