The galaxy exhibits an elliptical morphology, appearing as a smooth, concentrated distribution of light with a discernible cigar shape. Its color profile indicates a dominant population of older stars, exhibiting a yellowish-red hue. The galaxy shows no apparent spiral arm structures or dust lanes. There is a slight asymmetry in the light distribution. The galaxy's structure suggests it has likely undergone significant dynamical evolution, possibly including past or ongoing merger events. Star formation is present, but the color profile and low overall levels of activity suggest a relatively low star formation rate. The overall appearance points to a mature, massive galaxy.
