The galaxy presents as a relatively smooth, centrally concentrated system, with minimal visible disk structure or spiral arms. Its overall shape appears somewhat elliptical or spheroidal. The color gradient suggests a population of older stars, with redder hues dominating the central region. There might be some very faint, blueish star formation regions near the outer parts of the galaxy, but they are not particularly prominent. There do not appear to be any signs of major merging events, although there could be some minor disturbances in the disk.
