The galaxy presents a somewhat diffuse and irregular morphology. It appears as an amorphous, centrally concentrated object with faint, extended features. There is little evidence of spiral arms or a well-defined disk structure. The galaxy displays a subtle color gradient, with a slightly bluer hue in the outer regions and a redder hue towards the center. This suggests a potential difference in stellar populations, with younger, bluer stars possibly dominating the outer regions and older, redder stars concentrated in the core. There are some subtle asymmetries and irregular structures, potentially indicative of past or ongoing interactions, or internal dynamical processes. There is no obvious dust lane or obscuring material.
