The galaxy presents as an elongated structure, its morphology appearing predominantly smooth. A bulge is present, but it is not particularly prominent. The overall shape suggests an elliptical or lenticular classification, with a high probability of being cigar shaped. There is no evidence of significant spiral arms, and the light is concentrated towards the center, fading towards the edges. The color profile exhibits a redder hue, indicative of an older stellar population, likely with ongoing low levels of star formation. There's no obvious indication of major merger activity, although minor disturbances cannot be ruled out.
