The galaxy presents as a relatively smooth, centrally concentrated object. Its shape appears largely spheroidal, with a notable lack of discernible spiral arm structure or a prominent disk. The galaxy exhibits a color gradient, with a brighter, yellowish core that fades into a redder halo. Subtle irregularities in the outer regions suggest minor disturbances, possibly due to past interactions. The galaxy shows evidence of ongoing star formation, with intermediate values indicating the presence of young, massive stars, although the rate is not exceedingly high. There are indications of a merger event at some point in the past, possibly a minor disturbance or complete merger.