The galaxy presents as a moderately bright, resolved object with an overall elongated, lens-like morphology, suggesting a possible lenticular or early-type spiral galaxy. The central region exhibits a yellowish-white concentration of light, indicative of an older stellar population and potentially a bulge component. Extending outward from the core is a faint, diffuse disk. Within the disk, some asymmetric features and possible disturbances are noted, which may be indicative of minor gravitational interactions with another galaxy. The galaxy's color profile transitions gradually from the yellowish center to a bluer hue in the outer disk, possibly due to the presence of more recent star formation in the spiral arms. No significant tidal tails or other major merger signatures are readily apparent.
