The galaxy presents as a slightly elongated, elliptical structure with a smooth light distribution. There appears to be a concentrated central bulge, characterized by a yellowish hue, indicating an older stellar population. Extending outwards is a fainter, more diffuse halo. There is an indication of a slight disturbance or irregularity in the morphology, potentially suggestive of a minor interaction or past merger event. Overall, the galaxy appears relatively quiescent, with little evidence of active star formation visible in the image, but is disturbed. 
