The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a mostly spheroidal shape, with little evidence of a disk structure or spiral arms. The galaxy's light distribution is dominated by older stellar populations, as evidenced by the reddish-orange hue. There is a lack of significant blue color, suggesting a low rate of ongoing star formation. The smooth morphology indicates that the galaxy is likely a well-relaxed system, potentially an early-type galaxy. There is no apparent sign of tidal tails, strong dust lanes, or major disturbances, suggesting the absence of recent major mergers or interactions with other galaxies. Overall, the galaxy appears as a mature, quiescent system with a high degree of central concentration.
