The galaxy appears as a moderately bright, elliptical or lenticular system. Its core is a concentrated region of luminous material, exhibiting a yellowish-white color indicative of an older stellar population. The central region gradually fades into a less concentrated halo that extends outwards. The overall form is mostly smooth and symmetrical, with a subtle elongation that suggests it may not be perfectly spherical. There is no strong evidence of spiral arm structures, dust lanes, or prominent star-forming regions based on this image, suggesting a relatively quiescent galaxy with low to moderate star formation. The light distribution suggests it is a relatively massive galaxy, with no signs of active merging or major disturbances in its morphology.
