The galaxy presents an overall smooth morphology, with a centrally concentrated light distribution. Its shape is elliptical, appearing somewhat elongated. The light profile indicates a relatively featureless structure, without distinct spiral arms or a prominent bar. The color suggests a population of older stars, though there might be a hint of recent star formation. There is no strong evidence of ongoing major merging activity, although the presence of a slight asymmetry could indicate a minor interaction or disturbance. The galaxy's structure is consistent with that of an early-type galaxy, perhaps an elliptical or lenticular galaxy.