The galaxy presents as a lenticular, cigar-shaped structure with a smooth, diffuse light distribution. There is a subtle color gradient along the major axis, transitioning from a slightly bluer hue in what appears to be the central region to a redder color towards the outer edges. This may indicate a population of younger stars in the central regions and older populations in the outer regions. The galaxy appears relatively undisturbed, with no obvious signs of major merger events or tidal features. Faint arms may be present, but are not well defined. There is a relatively low rate of star formation. Overall, the galaxy appears to be a relatively evolved system.
