The galaxy presents an overall elliptical morphology, appearing somewhat flattened. A bright central bulge is visible, characterized by a concentrated luminosity. The galaxy exhibits a smooth appearance, but the suggestion of a disc component. This object appears to have undergone no major mergers recently. There is evidence of recent star formation. The spiral structure appears to be relatively symmetrical. The colour profile suggests a population of both older, redder stars, and bluer, younger stars.
