The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The light distribution is dominated by a yellowish-white core, indicative of an older stellar population. The outer regions display a fainter, bluer hue which implies the presence of younger stars, but the low intensity of these regions suggests a relatively low star formation rate. There are no obvious spiral arm structures or significant dust lanes visible. Overall, this galaxy appears to be an early-type spiral or lenticular galaxy with a dominant bulge and a subdued disk.
