The galaxy presents as an elongated, spindle-shaped object, displaying a generally smooth morphology with a possible disk-like structure. There appears to be a central bulge exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. Extending from the central bulge are fainter, bluish-tinted regions, potentially suggesting the presence of younger, hotter stars and some star-forming regions. The galaxy's overall shape suggests a classification leaning towards an elliptical or lenticular type, with some hints of a possible spiral component, albeit heavily obscured by the viewing angle and distance. There are no readily apparent signs of major mergers or significant tidal disturbances, however some minor disturbances cannot be ruled out.
