The galaxy appears to be a luminous, centrally concentrated object. It exhibits a largely smooth morphology with a subtle, diffuse halo. The core region shows a yellowish-white hue, suggesting an older stellar population. A slight blue tint is visible in the outer regions, potentially indicating ongoing, albeit subdued, star formation. There is no obvious spiral arm structure. The overall shape is approximately round, with only a minor deviation towards elongation. There is no clear evidence of any major merger activity or significant tidal disturbances in the immediate vicinity.
