The galaxy presents a largely smooth and rounded morphology. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core, with very faint hints of what could be a disk structure, though any spiral arms are not clearly delineated. The overall color profile indicates that the galaxy is most likely an elliptical, potentially of type E0-E3, viewed close to face-on. There is no obvious evidence of recent merger activity or significant tidal disturbances in the immediate vicinity of the galaxy.
