This galaxy presents as a relatively compact, smooth object. Its shape is generally round. There is little evidence of strong spiral arm structure or bar features. The galaxy appears to be dominated by an older stellar population, indicated by the yellowish hue of its central region, suggesting lower rates of recent star formation. There may be some very faint, bluer regions associated with the outer edges. There is no obvious indication of any ongoing major merger activity or significant tidal disturbances.
