The galaxy presents as an elongated, cigar-shaped morphology. It appears relatively smooth, with a concentrated central bulge that exhibits a yellowish hue, suggestive of an older stellar population. Extending from the central bulge are fainter, bluish arms or regions that may indicate more recent star formation. There is no apparent presence of spiral arms. Faint indications of dust lanes or patchy regions can be seen within the extended disk. The overall structure is generally undisturbed, with no obvious signs of a major merger event or tidal disruption.
