The galaxy appears to be an elliptical type, with a centrally concentrated bulge. The light distribution suggests a relatively smooth morphology, with minimal evidence of spiral arm structures or significant dust lanes. The galaxy is primarily yellowish-white in color, indicating an older stellar population, where star formation is either minimal or has ceased altogether. The elongation suggests an E4 or E5 classification on the Hubble sequence. There are no apparent tidal tails or distortions, indicating that the galaxy is not undergoing a major merger. The light is more concentrated in the center and fades as you get further from the center.
