The galaxy presents a generally smooth, elliptical morphology. Its light profile is concentrated towards the center, exhibiting a yellowish hue, suggesting an older stellar population. There is no prominent dust lane or spiral arm structure visible. A fainter, blue region is observed that may be a possible region of star formation, but appears to be a faint region of a spiral arm. Overall, the galaxy appears largely undisturbed, with no clear signs of major mergers or significant tidal disruptions.
