The galaxy presents a somewhat elliptical morphology, exhibiting a central bulge region with a concentrated core. There appears to be an extended disk, although its features are somewhat indistinct in this image. A smooth distribution of light is observed across the galaxy, which could indicate that a substantial fraction of the stars are in an older population. A faint blue hue is detectable, suggesting the possibility of ongoing, albeit subdued, star formation, particularly in the outer regions. The overall structure implies a degree of dynamical maturity and potentially indicates recent, minor interactions. The estimated size is small. There is some indication of minor disturbances.