This galaxy appears to be undergoing a significant gravitational interaction, potentially a merger or tidal disruption event. The morphology exhibits an elongated structure, possibly a tidal tail, extending from a brighter, more compact region. The brighter region shows an irregular shape and a central concentration of light, indicating the presence of a bulge or core. There is an evident color gradient across the galaxy, with bluer hues concentrated in the less dense, distorted regions, suggesting active star formation in those areas. In contrast, the central core displays a redder color, implying a population of older stars. The overall structure suggests a system that is not relaxed and is far from equilibrium. The absolute magnitude indicates that this is an intermediate luminosity galaxy. Low star formation rate, in particular low specific star formation rate, suggests that the rate of star formation is low compared to its stellar mass.
