The galaxy exhibits a generally smooth morphology, with minimal discernible features. The central bulge is prominent, displaying a concentrated, bright yellowish-white color, suggesting an older stellar population. Moving outwards from the core, the galaxy gradually fades into a more diffuse halo, with a slight flattening along its periphery. There is a subtle color gradient, with the outer regions appearing marginally bluer compared to the core, potentially indicating pockets of younger star formation, although limited in extent. The overall structure appears relatively undisturbed, with no clear evidence of tidal tails, mergers, or significant spiral arm structures. It appears to be a relatively isolated galaxy within its immediate environment. The object’s roundness suggests it may be close to face on. 
