The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated, with a radial decrease in surface brightness suggesting a lack of significant spiral arm structure or prominent star-forming regions. The color index, inferred from the DESI bands, suggests a population of older stars, potentially dominated by red giants and lower-mass main-sequence stars. This is typical of early-type galaxies with relatively low star formation rates. There is little evidence of tidal disturbances or ongoing merger activity in the immediate vicinity. The galaxy exhibits a moderately round shape, deviating slightly from a perfect circle, but it does not appear elongated or highly irregular. The estimated size, implies a moderate physical extent.
