The galaxy appears to be an early-type spiral or lenticular galaxy, presenting a relatively smooth, diffuse profile. The central bulge is prominent and appears somewhat elliptical in shape. There is some evidence of a faint, extended disk surrounding the bulge, though it lacks distinct spiral arm structure. The galaxy appears to be undergoing a minor interaction, or has possibly experienced a recent minor merger event, as there are some irregularities and a hint of tidal features present. The core regions emit a stronger green and orange spectral presence with what looks to be red spectral emissions in the disk, suggesting possible differences in stellar populations or ongoing star formation in these distinct regions. The galaxy exhibits a low rate of star formation and is moderately massive.
