The galaxy presents as a lenticular or possibly an elliptical morphology, exhibiting a smooth overall structure with little to no visible spiral arm features. It has an elongated shape, appearing cigar-like, suggesting it is viewed at an oblique angle. The central bulge is bright and prominent, with a yellowish-white hue, indicating a population of older stars. A fainter, bluish disk surrounds the bulge, implying the presence of some younger stars and ongoing star formation. The color gradient transitions from warmer tones in the center to cooler tones towards the outer edges. There may be some minor disturbances in the galaxy's shape, but no major interactions or mergers are apparent.
