The galaxy presents as a lenticular, cigar-shaped system with a smooth, relatively featureless morphology. It exhibits a bright, concentrated central bulge, appearing yellowish-white in color, suggesting an older stellar population. Surrounding the bulge is a diffuse, bluish halo that is elongated along the major axis, indicative of a disk component containing younger, bluer stars. There is no apparent spiral structure, nor any signs of significant tidal disturbances or ongoing mergers. The galaxy appears relatively isolated and undisturbed, suggestive of a settled evolutionary state. The estimated size is approximately 4 kpc in radius. Star formation is occurring at a rate typical for galaxies of similar mass.
