The galaxy appears as an elliptical or lenticular system, exhibiting a flattened spheroid shape. There is a dominant, luminous central bulge. The galaxy exhibits a primarily yellowish hue, indicating a population of older stars, with a possible absence of significant recent star formation. Faint blue tinges can be observed in the outer edges of the galaxy, which might represent sparse pockets of younger, hotter stars. The overall morphology suggests a system that has largely exhausted its gas supply. The galaxy is showing signs of a potential minor merger event and some disturbance in its structure.
