The galaxy appears to be a relatively luminous, elongated system, exhibiting characteristics of both elliptical and spiral morphologies. A central bulge region, slightly reddish in color, dominates the core. Extending outwards from this core is a faint, bluish disk-like structure, suggesting the presence of some recent star formation. The disk appears somewhat disturbed, with asymmetries in its shape and luminosity distribution. There's evidence of a possible interaction or merger event in the relatively close past, perhaps a minor interaction. The overall color indices suggest a mixed stellar population, with both older, redder stars in the bulge and younger, bluer stars in the disk. There also may be low-level star formation occurring within the galaxy. The luminosity profile is brighter in the green and red bands, and is quite luminous with a redshift of 0.098278. The overall shape of the galaxy is roughly a cigar shape. 
