The galaxy presents a somewhat elliptical morphology, appearing largely smooth in structure. A dominant central bulge is observed, exhibiting a yellowish hue suggesting an older stellar population. Fainter, less defined outer regions extend from the core, with a gradual decrease in surface brightness. There is a possible interaction or tidal disturbance visible towards the upper left of the galaxy's core, where a separate, less defined mass appears nearby. No distinct spiral arm structures or dust lanes are readily apparent, and the overall color profile indicates a relatively low rate of ongoing star formation. The galaxy displays a moderately compact appearance. A significant fraction of the light is concentrated in the core region.
