The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The galaxy appears to have minimal discernible disk-like structure or spiral arms. The light distribution suggests an evolved stellar population. No prominent dust lanes or active star-forming regions are readily apparent in this image. The galaxy's color is primarily a result of evolved redder stars with lower metallicities. The overall shape appears elongated. No signs of major tidal disturbances or ongoing mergers are immediately evident, although minor disturbances may be present.
