The galaxy exhibits a distinct elongated, cigar-shaped morphology. It presents a smooth, centralized bulge region that graduates outwards to a fainter, more diffuse disk. The overall color gradient transitions from a yellowish-orange hue in the core, suggestive of an older stellar population, to a bluer tint towards the outer regions, possibly indicative of ongoing star formation. The disk appears to be inclined at a significant angle relative to our line of sight. There is a slight asymmetry in the outer regions of the disk, indicating a possible minor disturbance or interaction.
