The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, appearing cigar-shaped rather than perfectly round. The light distribution within the galaxy is fairly uniform, lacking prominent spiral arms or a distinct central bulge. There may be signs of minor disturbances or interactions, possibly indicating a past or ongoing merger event, though no major tidal tails or dramatic distortions are readily apparent. The color profile suggests a relatively evolved stellar population, with a general redder hue implying older stars and less active star formation. Based on the color and smoothness, the system looks likely to be a massive galaxy, with the majority of stars being older.