The galaxy presents a somewhat amorphous, diffuse morphology. There is a central concentration of light, suggesting a bulge or core region. Extending outward, the light distribution is irregular and somewhat clumpy. There is a suggestion of tidal features or faint extensions, potentially indicative of past or ongoing interactions or mergers, making it more likely that it is interacting with another galactic body. The light is centrally concentrated, possibly suggesting the presence of an older stellar population. Based on the color gradient, a low star-formation rate is suspected. Overall, the galaxy appears to be a system with a relatively low level of internal organization and a moderately high stellar mass.
