The galaxy presents an elongated, cigar-shaped morphology. It appears to have a relatively smooth structure, with a possible central bulge region exhibiting a warmer, reddish hue, suggesting a population of older stars and/or dust obscuration. Extending outward from the central region, there is evidence of a bluer, more diffuse component, possibly indicative of younger stellar populations and ongoing star formation within a disk-like structure. There is a slight asymmetry to the outer regions of the galaxy, hinting at a possible gravitational interaction or minor disturbance event. Overall, this galaxy displays characteristics of a disk galaxy with an intermediate level of star formation.
