The galaxy presents a generally elliptical morphology. The central region exhibits a high surface brightness, appearing as a concentrated spheroid with a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the light gradually diminishes, suggesting a smooth transition into a more diffuse halo. There's a slight asymmetry in the outer regions, with a minor extension on one side, but no clear spiral arm structures or strong dust lanes are visible. The overall color profile suggests a relatively quiescent galaxy with limited ongoing star formation.
