The galaxy presents as an elongated, cigar-shaped structure. Its morphology appears relatively smooth, with a central bulge region exhibiting a yellowish-orange hue, possibly indicating a population of older stars. Fainter, bluish diffuse light surrounds this central region, potentially indicating some ongoing star formation within a disk component. There is no obvious indication of strong spiral arm structure or significant dust lanes. There might be a minor disturbance in the galaxy's overall shape, but it is not obvious. The galaxy is likely a spiral or lenticular type, seen edge-on. Its color profile suggests a considerable stellar mass.