The galaxy presents a generally smooth, elliptical morphology with a high degree of roundness. A slight elongation is observed, though the overall shape is not highly distorted. There is a clear central bulge that dominates the light profile, appearing as a concentrated, brighter region. The galaxy appears to be composed primarily of older stellar populations, as indicated by its overall yellowish-red color. There is no strong evidence of significant ongoing star formation within the galaxy from these colors, though some may still be occurring at low levels. Faint, extended emission is detected around the central region, likely comprising the galaxy's halo. There may be some very minor disturbances, but no signs of any major merging events or interactions with other galaxies are visible.
