The galaxy appears to be a relatively compact object, exhibiting a disk-like structure, though not perfectly circular. Its overall color profile suggests a population of older stars, with a subtle blue tint in some regions, implying ongoing though potentially subdued star formation. The morphology leans towards a smooth appearance, but with slight irregularities and features, hinting at potential past interactions or internal dynamics. The shape is somewhat elongated but not excessively so. There is no clear evidence of a major ongoing merger, although subtle disturbances might suggest minor tidal interactions in its history. Overall, this appears to be a galaxy that has settled into a more quiescent state, but retains subtle signatures of a dynamic past.
