The galaxy presents an elliptical morphology, appearing as a diffuse, luminous object with a brighter central core. The light distribution suggests a relatively smooth structure, with little indication of spiral arms or distinct features. There is some evidence of a faint extended halo surrounding the central region, indicating a broader distribution of stars and gas beyond the main body of the galaxy. Color gradients within the galaxy are subtle, the core of the galaxy appears bluer relative to the slightly redder outer regions. The overall structure shows signs of possible tidal disruption or minor interaction with another galaxy, suggested by asymmetry and a slightly irregular shape in the outer regions of the galaxy. There is no evidence of a major merger event currently underway.
