The galaxy presents a generally smooth, elliptical morphology. It is elongated, appearing more "in between" round and cigar-shaped, rather than distinctly spherical. The central bulge exhibits a concentrated, brighter luminosity, suggesting a high stellar density, and appears yellowish, potentially indicative of an older stellar population. A fainter, bluish halo surrounds the bulge. This could signify the presence of younger stars or ongoing, albeit subdued, star formation within the galaxy's outer regions. There's no clear evidence of strong spiral arm structures or a major ongoing merger event, though a possible minor disturbance cannot be ruled out. Overall, the galaxy seems to be a relatively quiescent, evolved system.
