The galaxy appears as a centrally concentrated, luminous object. Its morphology is largely smooth and featureless, lacking prominent spiral arms or a distinct bar structure. The light distribution suggests a roughly elliptical or spheroidal shape, with a gradual decline in intensity from the core outwards. Color gradients are subtle, with a slightly bluer core transitioning to a redder halo. No obvious signs of recent major mergers or tidal disturbances are evident. Star formation is likely present, as the galaxy is a bluish hue. There seems to be some indication of a faint disk. Overall, the galaxy resembles a relatively quiescent system, likely dominated by an older stellar population in its outer regions.