The galaxy presents a moderately elongated morphology. Its central region exhibits a high surface brightness, appearing smooth and relatively featureless, with a yellowish hue suggesting an older stellar population. Proceeding outwards, a fainter disk is observed, displaying a slight bluish tint, possibly indicating regions of ongoing star formation, although the color is subtle. The overall structure appears relatively undisturbed, lacking prominent signs of tidal interactions or major mergers. The shape tends more towards an elliptical form, yet it is not perfectly symmetrical. The galaxy appears to be a relatively isolated object based on the absence of nearby interacting galaxies. 
