This galaxy exhibits a somewhat elliptical morphology, appearing mostly smooth with a high degree of central concentration. There is some evidence of a minor disturbance or interaction occurring, possibly a merging event. One side of the galaxy presents a slightly elongated structure that may be the beginning of a tidal tail formation. The galaxy's color profile indicates a redder core, suggesting an older stellar population, while the outer regions show bluer hues, potentially indicating ongoing star formation or a younger population of stars. This galaxy is likely a massive system. The overall shape indicates it falls between a perfectly round and an elongated form.
