The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color profile suggests an older stellar population, with a dominant yellow-red hue in the core. The galaxy exhibits an approximate spheroidal shape, with only a slight deviation from perfect roundness. There are no visible signs of strong spiral arm structure or significant dust lanes. Faint, diffuse extensions are potentially visible on one side of the galaxy, indicating a possible minor tidal disturbance or interaction. The galaxy is exhibiting a low rate of star formation.
