The galaxy presents a generally smooth morphology, with a dominant spheroidal component. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light distribution indicates a centrally concentrated bulge.

Subtle color gradients are observable. The core exhibits a bluer hue that transitions to redder tones towards the outskirts. This may indicate varying stellar populations, with younger, bluer stars concentrated towards the galaxy's center and older, redder stars more prevalent in the halo.

There are hints of minor disturbances in the galaxy's overall shape. There may be slight tidal tails or asymmetries, suggesting potential past interactions or ongoing minor mergers.