The galaxy presents as a relatively compact, yet not perfectly smooth object. There is evidence of a central bulge, with a yellowish-white hue, suggesting an older stellar population. Fainter, bluer features are discernible, possibly indicative of more recent star formation occurring in the outer regions. The galaxy appears to exhibit some degree of disk-like structure, although it is not sharply defined. There is a hint of interaction, potentially a minor disturbance.
