The galaxy presents as an elongated, cigar-shaped structure, viewed at a significant angle relative to its apparent major axis. The light distribution suggests a relatively smooth morphology, with a central concentration of light that fades gradually towards the outer regions. The core appears to be yellowish-white, hinting at a population of older stars. The galaxy's light transitions to redder hues at the extreme ends of the major axis, possibly indicative of dust lanes or regions of ongoing, localized star formation. There is some asymmetry in the outer regions, hinting at a minor gravitational disturbance. Based on its morphology, the galaxy is likely an elliptical galaxy.
