The galaxy presents a smooth, elongated morphology, appearing cigar-shaped in visual inspection. Its light profile suggests a relatively homogenous stellar population, lacking prominent spiral arms or distinct features. A slight central concentration is observed, potentially indicating the presence of a galactic bulge. There is no apparent evidence of active galactic nuclei activity or significant dust lanes. The galaxy's color indices suggest a bias towards redder wavelengths, inferring an older stellar population and a comparatively low star formation rate. Overall, the galaxy appears as a relatively undisturbed, evolved system with a predominantly spheroidal structure.
