The galaxy appears to be a luminous elliptical, exhibiting a smooth, concentrated profile with a bright central bulge. Its overall shape leans towards round, but with some elongation. There is a subtle disk that is very faint. No spiral arm structures are discernable within the limits of the image resolution. There seems to be minor tidal disturbance present. The galaxy possesses a yellowish hue, suggesting an older stellar population with less ongoing star formation. Faint dust lanes or irregular features are observed, hinting at minor internal activity or a past interaction, although these could also be artifacts of the image. There may have been a possible merger in the past. The luminosity decreases steadily away from the core, with no distinct outer edge apparent.