The galaxy appears as a centrally concentrated object with a smooth light distribution. The core exhibits a yellowish hue, suggestive of an older stellar population. Fainter, diffuse light extends outwards from the core, displaying a subtle transition to redder colors in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology is relatively featureless, and the galaxy appears to be largely undisturbed. There might be some minor disturbance that could be causing some star formation. 
