This galaxy exhibits a generally smooth morphology, with a centrally concentrated light distribution. While a disk cannot be entirely ruled out, the overall appearance suggests a likely classification as an elliptical galaxy. There is a faint, diffuse halo surrounding the central bulge. Evidence of minor disturbances is visible in the form of some faint asymmetric light in the outer regions, which may indicate past or ongoing interactions with another galaxy. While there are no clear spiral arms, a very faint, almost indiscernible disk-like structure is weakly suggested. There are no bright, well-defined star-forming regions apparent; the overall color suggests an older stellar population with little current star formation.
