The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated luminosity, suggestive of a substantial stellar population or active galactic nucleus activity. The light profile appears smooth, lacking prominent spiral arm structures or distinct dust lanes. There's a subtle color gradient with the core appearing more yellow, while the outer regions show a slight bluer hue, indicating the presence of younger stars or differing stellar populations. The galaxy's smooth light distribution and shape are consistent with an elliptical classification, though a highly inclined disk galaxy cannot be entirely ruled out without further spectral analysis. Subtle asymmetric features may indicate ongoing or past interactions with another galaxy.
