The galaxy appears to be a luminous, elliptical galaxy, exhibiting a smooth, spheroidal morphology. There is a concentration of light toward the center. No distinct spiral arm structures or prominent dust lanes are visible. There seems to be a slight elongation. The galaxy displays a yellow/orange hue, suggesting an older stellar population. The system's mass appears substantial, characteristic of a galaxy residing within a group or cluster environment. There's evidence of possible ongoing or past minor interactions, given the slight disturbances.
