The galaxy presents a largely smooth morphology, with minimal discernible features such as spiral arms or a prominent disk structure. The light distribution suggests an elliptical or lenticular form, characterized by a centrally concentrated bulge that fades gradually towards the outer regions. The color appears to be predominantly yellow-reddish, potentially indicative of an older stellar population with lower ongoing star formation. The overall rounded shape contributes to the impression of a well-established, relatively quiescent system. There is no obvious evidence of any major merger events or significant tidal disturbances affecting its structure. Faint hints of bluer light are present in its outer reaches, suggesting a potential for younger stars existing in the galaxy.
