The galaxy presents an elongated, cigar-shaped morphology. The primary axis of the galaxy displays a yellow-orange hue, suggesting a population of older stars and/or dust obscuration. Fainter blueish light is visible towards both ends of the major axis, possibly indicative of some low-level ongoing star formation within the galaxy. The object does not appear to possess any distinct spiral arm structure or a well-defined central bulge. Overall, the galaxy appears to be relatively smooth, with no strong indications of significant mergers or tidal disturbances in its immediate vicinity. The galaxy's color profile suggests a population of older stars with some regions of ongoing or recent star formation. The light from the galaxy is moderately redshifted, indicating that it is at a significant cosmological distance.
