The galaxy presents as a luminous object with a notable central concentration of light. The morphology appears to be generally smooth with a slight elongation, possibly indicative of an elliptical shape or a disk galaxy viewed at an angle. There is some evidence of internal structure, but the resolution limits a more detailed assessment. The galaxy exhibits a color gradient, appearing yellower in the central region and slightly bluer towards the outer edges, suggesting a distribution of stellar populations with older stars centrally located. The galaxy's profile suggests a relatively high mass and correspondingly low specific star formation rate. There does not appear to be any ongoing merger events, but there is some visible disturbance.
