The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a concentrated, bright core, displaying a yellowish hue. Extending outwards, the galaxy shows a more diffuse and slightly bluer outer structure, suggesting ongoing or recent star formation in these regions, although this star formation seems fairly subdued. Patches of redder color are present within the disk, possibly indicating areas of dust obscuration or older stellar populations. There is some evidence of minor disturbances or asymmetries in the galaxy's structure. Overall, the galaxy appears as a somewhat disrupted system with a dominant spheroidal component and a fainter, less organized disk.