The galaxy presents as a roughly elliptical morphology with a smooth light distribution. Its central region exhibits a high surface brightness, appearing bright yellow-white in color, suggesting a concentrated stellar population. Moving outward, the light gradually diminishes, transitioning to a diffuse, faint bluish halo. There appears to be minimal evidence of spiral arms or a prominent disk structure. No significant dust lanes or tidal features are readily discernible, indicating a lack of recent major merger events. It appears relatively undisturbed, displaying no distinct signs of active star formation regions in the visible spectrum.
