The galaxy presents an elliptical morphology, exhibiting a relatively smooth and diffuse light profile. It appears generally round, although a slight elongation is observed along a single axis. The central region of the galaxy displays a strong concentration of light, with a color index tending toward redder wavelengths, suggesting a population of older stars. Fainter, bluer regions are observed asymmetrically around the core and suggest star forming regions. There appears to be a gravitational disturbance in the image, maybe indicating a collision with another galaxy.
