This galaxy appears to be a relatively small, elongated system with a smooth morphology. The light distribution suggests a central bulge that gradually fades towards the outer edges. The galaxy exhibits a faint disk-like structure, characterized by a slightly bluer color compared to the central regions, hinting at the presence of ongoing or recent star formation activity within the disk. There are no apparent signs of spiral arms or prominent dust lanes, and no indications of any major ongoing merger events or significant tidal disturbances. The galaxy's overall color suggests a mix of stellar populations, with a possible dominance of older stars in the central bulge and a younger population contributing to the blueish tint in the disk. The galaxy appears to be relatively isolated.
