The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. There is a noticeable radial color gradient, transitioning from a yellowish core to a bluer outer region. The overall morphology suggests a system with a dominant spheroidal component. The apparent lack of distinct spiral arms or prominent dust lanes points towards a galaxy with a less active star formation rate. The light distribution appears largely uniform, with no significant evidence of major tidal disturbances or ongoing merger events.
