The galaxy presents an overall elliptical morphology, elongated with a cigar-shaped appearance. The central region exhibits a yellowish-white hue, indicative of an older stellar population and/or dust obscuration. The outer regions display a reddish-orange tint suggesting the presence of dust and possibly cooler, older stars. A subtle blue-greenish tinge is observed within the disk, possibly indicating localized regions of ongoing star formation. The galaxy appears relatively smooth, with no strong evidence of spiral arms or major morphological disturbances. There are no apparent signs of a major merger. The overall structure suggests a galaxy in a relatively quiescent state.
