The galaxy presents a largely smooth morphology, appearing nearly spheroidal in shape. There is little evidence of spiral arms or significant disk structure. The light distribution is concentrated towards the center of the galaxy, suggesting a prominent bulge. The galaxy exhibits a color gradient, with the central region appearing slightly redder than the outer regions. The overall color index suggests a population dominated by older stars. There are no obvious signs of ongoing major mergers or tidal disturbances, although a very slight asymmetry could indicate a minor interaction in its past. The galaxy appears to be relatively isolated.
