The galaxy presents as a relatively smooth, amorphous structure, exhibiting an elliptical morphology. Its light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The galaxy exhibits a yellow-orange hue, suggestive of an older stellar population with a low rate of ongoing star formation. There is evidence of a possible merger or tidal interaction, indicated by a slight distortion in the galaxy's overall shape and a secondary concentration of light near the main body. The galaxy displays a roundness with a small degree of disturbance in its morphology. Overall, the galaxy appears to be a massive elliptical undergoing some level of interaction.
