The galaxy presents a smooth, elongated morphology, with an approximate effective radius of 10.5 kpc. Its central region exhibits a bright, concentrated core, which diffuses outward into a more indistinct and diffuse halo. The galaxy’s overall shape is somewhat cigar-shaped, and there is little evidence of prominent spiral arm structures or a well-defined disk. The light distribution is relatively even across the main body of the galaxy, without large clumps or strong irregularities, although some faint features and minor disturbances are present. The overall color is predominantly yellowish, suggestive of an older stellar population. Star formation appears to be present but is occurring at a low rate. No signs of a recent major merger are apparent; the galaxy appears relatively undisturbed.
