The galaxy presents a generally smooth morphology. It exhibits a centrally concentrated bulge with a yellowish hue, suggesting a population of older stars. Surrounding the bulge is a fainter, somewhat flattened disk. The disk appears bluish-green, potentially indicating the presence of younger, hotter stars and ongoing star formation, albeit at a relatively low rate. The galaxy displays a moderate ellipticity, appearing somewhat elongated. There is no clear evidence of major disturbances or interactions with other galaxies. The estimated size of the galaxy is approximately 4 kiloparsecs in radius. The estimated red shift suggests it is relatively distant.
