The galaxy presents as a moderately bright, somewhat elongated elliptical shape. A prominent central bulge exhibits a smooth, concentrated luminosity, displaying a yellowish-orange hue. This central region appears largely featureless at this resolution. The outer regions of the galaxy fade gradually, exhibiting a diffuse, less concentrated distribution of light. Hints of bluer tones are visible in these fainter, extended regions, potentially indicating the presence of younger stellar populations relative to the core. There is no apparent spiral structure or dust lane visible. The overall appearance suggests a relatively evolved system. No obvious signs of tidal interaction or significant morphological disturbance are detected.
