The galaxy appears as a centrally concentrated object with a generally smooth morphology. The central region exhibits a yellowish hue, possibly indicative of an older stellar population dominating the core. There is a subtle decrease in the brightness moving outwards from the core. No distinct spiral arms or bar structures are readily apparent. The overall shape seems approximately circular, with minimal elongation. The observed colour suggests relatively low levels of recent star formation. There is no indication of any major mergers or significant tidal disturbances. Minor irregularities are hard to asses, but there are no indications of any.
