The galaxy presents a smooth, elliptical morphology. It exhibits a central bulge that appears relatively bright and concentrated. The galaxy's overall shape is elongated, with a cigar-like appearance rather than a perfectly circular form. There is little evidence of distinct spiral arms or significant star formation regions. The color profile suggests a population of older stars, leading to a more reddish-yellow hue within the central region. The outer regions fade into a less defined halo, showing a gradual decrease in stellar density and overall luminosity. There is no indication of ongoing major mergers, although there might be very minor signs of disturbance present.
