The galaxy presents as a centrally concentrated, relatively smooth object with a noticeable color gradient. The core region exhibits a yellow-gold hue, suggesting an older stellar population. Moving outward from the core, there is a transition to a bluer color profile. This is likely due to more recent or ongoing star formation in the outer regions of the galaxy. There's no apparent spiral structure, and no distinct galactic bar. The overall shape appears to be relatively round. There's a suggestion of some minor disturbance or asymmetry in the galaxy's halo, indicating possible past interactions or accretion events. However, it does not present as a major merging event. 
