The galaxy presents as an elongated, cigar-shaped structure, likely an edge-on or highly inclined disk galaxy. A bright, concentrated central bulge is visible, suggesting a significant population of older stars. The disk appears relatively smooth, with a general lack of distinct spiral arm structure, but some slight colour variations suggest differential stellar populations. The colour profile suggests that the bulge is more composed of older, redder stars and the disk has slightly bluer regions, likely indicating some ongoing star formation. Overall, the galaxy appears to be a moderately massive system with a relatively quiescent star formation rate.
