The galaxy presents as an elliptical system, possibly an early-type spiral seen at an oblique angle. The central bulge is prominent and exhibits a smooth, concentrated luminosity profile. The overall color suggests an older stellar population, with a somewhat subdued blue tinge indicating that some younger stars might exist. The disk appears relatively undisturbed, with no significant evidence of tidal features or ongoing major mergers. There's a potential hint of a faint spiral structure, but the image resolution makes it difficult to confirm definitively. The galaxy's apparent roundness suggests a later-type elliptical or a face-on spiral galaxy. There are some minor asymmetric features, possibly indicative of minor disturbances but the galaxy is, for the most part, relaxed and undisturbed. Overall, it appears as a moderate-mass galaxy with a low star-formation rate and residing at a redshift of approximately 0.116, placing it at a substantial distance.
