The galaxy presents as a slightly elongated, elliptical structure with a smooth, diffuse appearance. A central bulge dominates the galaxy's morphology, exhibiting a bright, concentrated luminosity. Moving outwards from the bulge, the light intensity gradually decreases, fading into the surrounding space. The color profile suggests an aging stellar population, with a yellowish-red hue indicating the presence of older, cooler stars. No distinct spiral arms or prominent dust lanes are visible. There is little evidence of recent star formation activity. The galaxy does not appear to be undergoing any major mergers or tidal disruptions. Based on these observed characteristics, the galaxy likely represents a mature, relatively quiescent elliptical galaxy.
