The galaxy appears to be a lenticular or possibly an elliptical galaxy, viewed at an oblique angle. It exhibits a generally smooth morphology with a bright, concentrated central bulge that dominates its overall luminosity. The light from the bulge is yellowish-white, suggesting an older stellar population. A faint, extended disk surrounds the bulge. This disk is not well-defined, appearing more like a gradual fading of light intensity rather than distinct spiral arms or prominent dust lanes. The galaxy displays a notable elongation, its shape deviates significantly from being circular. The major axis is several times longer than the minor axis. Some evidence exists for possible tidal debris or faint extensions along the major axis, particularly at one end of the galaxy, hinting at past interactions. Overall, the galaxy's color suggests a population of older stars and low ongoing star formation, typical of early-type galaxies.
