The galaxy presents a flattened, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's core, exhibiting a yellowish-white hue, suggesting a population of older stars. Surrounding the bulge is a fainter, bluish disk component, which is elongated and oriented horizontally in the image. The disk shows some subtle variations in surface brightness, but no distinct spiral arm structure is discernible. There appears to be a slight warping or irregularity in the shape of the outer disk, possibly indicative of a minor gravitational interaction. Overall, the galaxy exhibits characteristics consistent with a late-type spiral, possibly transitioning towards an S0 morphology due to its prominent bulge and relatively smooth disk. Star formation appears to be present, but not dominant within the galaxy, concentrated mainly within the disk. There is no evidence of a major ongoing merger.
