The galaxy presents a somewhat amorphous, yet discernible disk-like structure, with a central bulge that appears bright and relatively smooth. The overall color profile suggests a mix of stellar populations. The presence of blue-ish hues scattered throughout the galaxy indicates ongoing or recent star formation, particularly along what appear to be faint, diffuse spiral arm segments. Conversely, the central bulge exhibits a yellow-reddish color, suggestive of an older stellar population. There's some indication of slight disturbances or asymmetries in the disk structure, potentially hinting at past or ongoing interactions with other galaxies or internal dynamic processes. The galaxy does not appear to be undergoing a major merging event, although small tidal features may be present.
