The galaxy presents as a slightly elongated structure, displaying a moderate degree of smoothness overall. The color profile suggests a mix of stellar populations. A brighter, yellowish central bulge is discernible, indicating a likely concentration of older, evolved stars. Fainter, bluer regions appear to extend outwards from the bulge, hinting at ongoing or recent star formation within a disk-like component. There is some indication of a possible minor tidal disturbance or interaction, with a faint, asymmetrical extension or arm-like feature. Based on its apparent morphology, it does not appear to be a late-stage merger. However, there may be some sort of interaction occurring, and the disk seems mildly disturbed.
