The galaxy presents a generally elongated morphology, appearing cigar-shaped. The light distribution seems to be mostly smooth and centrally concentrated, implying that it may be of an elliptical nature. The core region exhibits a yellowish-orange hue, potentially indicating an older stellar population. Fainter, bluer light is visible in a more concentrated region slightly offset from the central bulge; this suggests the possibility of star formation. The galaxy does not present any obvious signs of major tidal disturbances or large-scale merging events.
