This galaxy appears as a somewhat elliptical, moderately luminous object. The light profile is relatively smooth, with a gradual decline in brightness from the center outwards. There is a subtle suggestion of a disk component, although it is not sharply defined. Some irregularity in the outer regions may indicate minor tidal disturbances or interactions. The galaxy exhibits a slightly bluish hue centrally, suggesting some ongoing star formation, with redder tones towards the periphery. Given its apparent size, it seems to be a dwarf galaxy with an estimated stellar mass of 10^8 solar masses. Star formation appears to be relatively quiescent, with a low star formation rate. There is no evident spiral structure or bar feature.
