This galaxy appears to be an elliptical type. The light profile is smooth and centrally concentrated, exhibiting a gradual decline in brightness from the center outwards. The isophotes appear moderately elliptical, displaying a ratio of major to minor axis of approximately 2 to 1. There is no evidence of distinct spiral arms or a prominent disk structure, suggesting a more spheroidal morphology. The color is generally homogenous, with a slight trend towards redder hues in the central regions, likely indicating an older stellar population. There are no indications of any ongoing major merger events or significant tidal disturbances. Marginal evidence exists for faint, diffuse extensions, but they appear indistinct.
