The galaxy presents as a concentrated spheroid of light, with a smooth, almost featureless appearance. The central region exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color shifts to a slightly bluer tone, indicative of more recent star formation within the galaxy's disk or outer regions. The overall shape appears somewhat elongated, but not significantly cigar-shaped. There appears to be a faint tidal tail on one side of the galaxy, although this could be a secondary galaxy and not a part of the main galaxy. There does not appear to be any significant evidence of a grand design spiral structure or other prominent features in the disk. The luminosity suggests a massive galaxy, likely with a substantial population of stars and a significant amount of dark matter. Star formation appears to be present but is likely occurring at a moderate rate.
