The galaxy presents as a relatively bright, somewhat centrally condensed object. Its morphology appears largely smooth, suggesting a possible elliptical classification or a spiral galaxy seen face-on with a prominent bulge. There is an observed extension or tidal feature to the south. The galaxy exhibits a color gradient, appearing bluer towards the central region and more yellow or red towards the outer regions and extension, indicating a potential difference in stellar populations. The relative smoothness suggests a well-mixed stellar population with potentially less active recent star formation in the central region, but the bluer core and bluer extension suggest some more recent star formation is happening within that region. The isophotes appear to be relatively round. There is no obvious evidence of ongoing major merger activity but the possibility of a minor interaction or past merger event is suggested by the extension.
