The galaxy presents as a relatively compact structure with a smooth overall appearance. Its color profile suggests a slightly higher concentration of older stars. There is evidence of some features or a disk-like structure that are present, but not overwhelmingly distinct. The galaxy exhibits a high degree of roundness. There might be some minor disturbances in the gravitational environment, with no strong evidence of a major ongoing merger. Star formation appears to be occurring at a moderate rate, and a relatively low specific star formation rate. The galaxy has an estimated mass on the order of 10^9 to 10^10 solar masses.
