The galaxy presents as a smooth, elongated structure. The central region exhibits a concentrated luminosity, suggesting a prominent bulge. Moving outward from the core, the light gradually diffuses into a less defined disk. The galaxy's color profile indicates a dominant population of older stars. The overall morphology suggests this galaxy is most likely an elliptical galaxy with a slight cigar shape, or perhaps an early-type spiral galaxy viewed at an oblique angle. There's no obvious signs of recent major merger activity, but there is a potential minor disturbance within the galaxy itself. The estimated size of this galaxy is approximately 4.3 kpc, indicating a relatively compact system. We observe that this galaxy is undergoing star formation.

