The galaxy presents a reddish hue, suggesting a population of older stars or significant dust obscuration. The morphological features include a slightly irregular shape with some subtle signs of disturbance, such as faint wisps or extensions emanating from the central region. There appears to be some underlying smooth component, however, this component appears disrupted by interactions.

Based on the overall features, this galaxy likely experienced some minor gravitational interaction or merging event in its past.
