The galaxy appears to be an elongated, likely disk-shaped structure seen at a significant inclination relative to our line of sight, possibly close to edge-on. Its central region exhibits a concentrated, relatively smooth luminosity profile, suggesting a possible bulge component. The light from the central region is somewhat redder in color than the outer regions, which hints at an older stellar population dominating the bulge. The disk itself is less well-defined, with a somewhat fuzzy appearance, which indicates a distribution of stars and dust. There appears to be a slightly lopsidedness to the disk's outer edges with hints of some faint extended structure beyond the main body of the galaxy. There is no obvious presence of bright, blue star-forming regions. The overall color profile suggests that it has undergone significant stellar evolution and may have a relatively low ongoing star formation rate. The galaxy seems to be relatively isolated, showing no strong signs of ongoing tidal interaction or merging events in this image.
