The galaxy exhibits a somewhat elongated, cigar-shaped morphology. It presents a central, concentrated bulge region that appears smooth and featureless in this image. The color profile suggests a dominant older stellar population within the bulge, indicated by the yellowish hue. Extending from the central bulge are faint, diffuse features that may constitute a rudimentary disk component. These features are less structured and less luminous than the bulge. The overall color gradients suggest some level of active star formation. There is no significant evidence of tidal features, major disturbances, or interaction with other galaxies in this field.
