The galaxy appears to be a relatively bright elliptical. Its color profile indicates an older stellar population, with a dominant reddish-orange hue at its core. This suggests a significant presence of evolved stars. The galaxy is largely smooth in appearance, lacking prominent spiral arms or significant dust lanes. There appears to be a very slight elongation of the galaxy's morphology. There may be a minor merger or tidal disturbance present, indicated by a faint and diffuse extension of light emanating from the main body. The overall light distribution appears concentrated towards the core.
