The galaxy presents as a relatively compact object. Its morphology appears largely smooth and elliptical. The light distribution is concentrated towards the center, with a gradual falloff in intensity towards the outer edges. There is a subtle color gradient visible, with a slightly bluer central region potentially indicative of ongoing star formation, transitioning to redder hues in the outer parts, which may suggest an older stellar population. There is no clear evidence of spiral arms, a bar structure, or significant tidal disturbances. The galaxy appears well-defined, with no signs of a major ongoing merger, although subtle irregularities may suggest minor past interactions. The overall structure suggests a galaxy that is relatively evolved and not undergoing violent processes of galaxy formation or destruction.
