The galaxy presents as an elliptical or lenticular system. It exhibits a relatively smooth light distribution, with minimal discernible substructure. There are no apparent spiral arms or a distinct central bar. The object appears significantly more luminous at its core, with a gradual decline in surface brightness towards the edges. The galaxy displays a notable yellow-red color profile, suggesting a population of older stars and a suppressed rate of recent star formation. The shape of the galaxy appears moderately elongated, tending toward a more circular morphology than a highly flattened one. There is no obvious visual evidence of any ongoing major merger activity or significant tidal disruption.
