The galaxy presents as a slightly elongated, cigar-shaped structure, with a dominant smooth component. It exhibits a color gradient, appearing reddish in the central regions, shifting to a more greenish-yellowish hue towards the outer edges. This color transition suggests a possible variation in stellar populations, with older, redder stars concentrated centrally and younger, bluer stars populating the disk. There is no distinct spiral arm structure visible, nor are there any obvious signs of a major ongoing merger event, though a very subtle asymmetry or minor disturbance cannot be entirely ruled out. The galaxy seems to be relatively isolated with no immediately apparent tidal features or companion galaxies interacting with it in this image. The overall morphology hints at a relatively quiescent system, possibly an early-type spiral or lenticular galaxy at an approximate distance corresponding to a redshift of around 0.2. Its estimated size is roughly 8 kpc in radius. Given the color profile, the galaxy is likely undergoing a low level of star formation.
