The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution with no readily apparent spiral arms or significant disk-like structure. The color gradient is subtle, suggesting an older stellar population with relatively little ongoing star formation. The galaxy appears moderately luminous, indicative of a substantial stellar mass. Its overall shape is largely spheroidal, deviating only slightly from a perfect circular form. There is no visual evidence of any major merger events or significant tidal disturbances affecting the galaxy's structure, although subtle asymmetries or minor disturbances cannot be entirely ruled out at this resolution.
