The galaxy presents as a diffuse, relatively compact object. Its morphology appears to be largely smooth, lacking any prominent spiral arm structure or a well-defined galactic bulge. The color profile indicates a slightly redder hue, suggesting a population of older stars and a lower rate of active star formation. There is no evidence of a recent major merger event, tidal tails, or other significant morphological disturbances. However, a minor asymmetry in the shape might indicate a past minor interaction. The general appearance aligns with that of an elliptical or lenticular galaxy with a considerable amount of its light concentrated toward the center.
