The galaxy presents as a centrally concentrated object with a generally smooth appearance. There is little indication of spiral arm structure or prominent dust lanes within the optical wavelengths observed. The light distribution exhibits a radial profile that appears relatively symmetrical, with a subtle elongation or asymmetry on one side. The core displays a yellowish-white color, suggesting an older stellar population, while the outer regions have a bluer hue, possibly indicating the presence of younger, hotter stars or ongoing star formation in the outskirts. Evidence of disturbance such as tidal tails or interactions are not apparent.
