The galaxy presents as a central, relatively smooth light distribution with faint extensions or tidal features suggestive of possible gravitational interaction or a recent minor merger event. The main body exhibits a slightly elongated morphology. The color profile across the galaxy appears relatively uniform, with a subtle shift towards redder hues in the central region compared to the outer edges. There is not a well defined disk, but there are minor disturbances in the light. There may be a faint, thin tidal tail extending from the galaxy, indicating ongoing or recent interaction. Based on these characteristics, the galaxy is likely an early-type spiral galaxy, although without higher resolution imaging, more detail could be found.
