The galaxy appears as a relatively small, lenticular or possibly early-type spiral system. Its overall shape is elliptical, with a high degree of central concentration of light. The luminosity profile is relatively smooth, suggesting a dominant bulge component. There is a subtle hint of a disk component, possibly exhibiting faint spiral arm structures, however, the resolution does not allow for a definite conclusion. The color is a relatively uniform bluish-white, indicating a moderate population of young, hot stars, but also a potentially significant population of older, redder stars, given the color indices. There might be indications of a minor disturbance or interaction, such as a slight asymmetry in the light distribution, but this is not conclusive. The galaxy appears to be relatively isolated, with no close companion galaxies visible in the immediate vicinity.
