The galaxy presents a largely smooth and rounded morphology, with a concentrated central region. The color profile suggests a relatively older stellar population. A subtle green tinge is visible in the halo, which could indicate recent, low-level star formation, though the bulk of the light appears to be from evolved stars. There is no indication of significant spiral arm structure or dust lanes. No interactions or tidal features are readily apparent, further supporting the conclusion that this galaxy is undisturbed. The galaxy exhibits an elliptical shape.
