This galaxy appears to be a somewhat elongated, lenticular or possibly an elliptical type, viewed at an oblique angle. The light distribution suggests a relatively smooth structure, with a brighter central region that could represent a galactic bulge or a higher density of stars and gas. The lack of clearly defined spiral arms indicates a likely absence of significant ongoing star formation. There is a slight asymmetry to the galaxy’s shape, with one edge appearing more extended or possibly perturbed, potentially hinting at past or ongoing gravitational interactions. There also may be an irregularity to the galaxy in the form of a tidal tail. Overall, the galaxy presents a generally smooth appearance, consistent with a lack of prominent features.
