This galaxy presents as a relatively faint object. It appears to be a disk galaxy, though without high-resolution imaging, the presence and structure of spiral arms are difficult to discern. The galaxy exhibits a centrally concentrated luminosity, which fades gradually towards its outer edges. The core region displays a slightly bluer hue compared to the outer regions. The overall color suggests a stellar population of mixed ages, with some ongoing or recent star formation activity. The object shows some irregularity in shape, which could potentially indicate a past or ongoing minor merger event.
