The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color appears to be yellowish-orange, suggesting a population of older stars. The light distribution seems largely homogenous without prominent spiral arms or distinct features, potentially indicating an elliptical or lenticular galaxy. There is a slight elongation in its shape, departing from a perfectly circular form. Based on the available data, the galaxy appears to be in a relatively quiescent state of star formation, and there is no evidence of major merger activity or tidal disturbances within the visible structure. It could potentially be an early type spiral, but does not readily present any clear spiral structure.
