The galaxy presents as a relatively elongated, disk-like structure. The central region exhibits a higher surface brightness and appears predominantly yellowish-white in color, suggesting an older stellar population. Moving outward from the core, the color shifts subtly towards a bluer hue, indicating the presence of younger, hotter stars. The overall structure appears smooth and regular, with little evidence of strong tidal disturbances or merging activity. There is a faint hint of spiral arm structure. The galaxy's apparent size is small, consistent with its classification as a distant object. The morphological characteristics of the galaxy suggest it is likely an elliptical galaxy, possibly with some disk galaxy features still visible.
