The galaxy presents as a slightly elongated spheroid, displaying a generally smooth morphology. A prominent central bulge region exhibits a brighter, more concentrated luminosity, transitioning into a fainter, less defined outer disk or halo. The color distribution suggests a mix of stellar populations; the central bulge appears relatively redder, indicative of older stars, while the outer regions show bluer hues, possibly suggesting the presence of younger stars or ongoing star formation. There is no distinct evidence of spiral arm structures, but subtle features or irregularities are observed. The galaxy appears relatively undisturbed, exhibiting only minor signs of potential tidal interactions or past mergers.
