The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing as a bright, reddish-orange core. Moving outward from the core, the light intensity decreases gradually. A faint, greenish-yellowish halo surrounds the central region, extending further along the major axis than perpendicular to it. The galaxy appears more elongated and cigar-shaped than perfectly circular. There is no visible evidence of spiral arms, prominent dust lanes, or major disturbances suggesting an ongoing merger. The overall morphology suggests a relatively evolved galaxy with a dominant bulge component and a less prominent disk. The redder color of the core indicates an older stellar population, while the greenish-yellowish halo might be indicative of some residual, lower-level star formation activity.
