The galaxy appears relatively smooth and compact, with a generally circular morphology. It exhibits a centrally concentrated brightness profile, suggesting a dominant bulge component. The galaxy's color is predominantly a blue-green hue, indicative of potential ongoing or recent star formation activity. No distinct spiral arms or bar structures are readily apparent. Faint extensions or asymmetries may be present, possibly indicative of minor tidal interactions or internal disturbances, but more data would be required to determine that with more certainty. 
