The galaxy presents a morphology that appears generally smooth, though with subtle features hinting at a disk-like structure. The luminosity is concentrated towards the center, suggesting the presence of a central bulge, possibly housing a supermassive black hole. The overall shape is somewhere between round and elongated, with a hint of a cigar shape. There is a possible minor disturbance, but otherwise the galaxy seems to be relatively undisturbed. The galaxy displays a primarily bluish color, which indicates it contains a substantial population of younger, hotter stars. The estimated mass of the galaxy is likely between 10^8 and 10^9 solar masses, placing it on the lower end of typical galaxy sizes. The relatively low star formation rate suggests that it may be in a transition phase towards a more passive state.
