The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. There is a subtle elongation, diverging from a perfectly circular profile. Faint, diffuse extensions emanate from the central region. The galaxy appears relatively isolated, without any obvious signs of major interaction with neighboring galaxies, although a small distortion is evident in its shape. The faint star-forming regions imply a low rate of current star formation activity. 
