The galaxy presents a generally smooth morphology, with a concentrated central bulge. The light distribution suggests a lack of prominent spiral arms or a well-defined disk structure. The galaxy exhibits a blue color profile, most prominent away from the bulge region, suggesting the presence of ongoing star formation. There is a faint indication of a disturbance or possible minor merger event, which could be contributing to the observed star formation. Based on its overall appearance, this galaxy appears to be an intermediate mass system, actively forming stars, and possibly undergoing a minor interaction.
