The observed galaxy exhibits a morphology suggestive of an elliptical or lenticular type, with a relatively smooth light distribution. The galaxy's shape appears more akin to an intermediate elliptical, exhibiting a moderate degree of ellipticity. The primary body of the galaxy displays a yellowish hue, potentially indicating an older stellar population. Evident is a disturbance within the galaxy. These disturbances could indicate past minor merger events, tidal interactions, or other gravitational perturbations. This is further suggested by the presence of blue emissions towards the left side of the galaxy, indicating the presence of younger stars. This may be due to interactions with another galaxy or tidal gas compressing to form new stars. The surrounding regions do not exhibit prominent spiral arms or a well-defined disk structure. This makes it difficult to determine whether the galaxy is actively undergoing significant star formation or whether it is dominated by an older, more quiescent stellar population. The galaxy displays an asymmetrical structure.
