The galaxy presents as a moderately inclined disk galaxy. Its overall color profile appears yellowish, suggesting a dominant population of older stars and a relatively low rate of on-going star formation. The central bulge region exhibits a bright, concentrated luminosity, and a smoother texture indicative of an elliptical morphology. The disk component is less clearly defined, appearing somewhat blurred with hints of spiral structure. The outer regions of the galaxy show a gradual decrease in brightness. There are no clear indications of significant tidal disturbances or major mergers. The galaxy is elongated in shape, with a ratio of approximately 3:1 of its major to minor axis.
