The galaxy presents an elongated morphology, with a smooth, centrally concentrated bulge. There is an indication of a disk component, though it appears relatively faint and unstructured. The galaxy exhibits a blue hue, particularly in the disk region, suggesting the presence of younger stellar populations and ongoing star formation. The object appears relatively isolated, without obvious signs of major interaction or ongoing merger activity, though there may be minor disturbances visible in the outer regions. The shape suggests a departure from a perfect spheroid, tending toward a cigar shape. The system's overall appearance is consistent with a spiral or lenticular galaxy, though the lack of well-defined spiral arms makes precise classification difficult.
