The galaxy presents a generally smooth morphology. Its shape appears largely spheroidal, exhibiting a high degree of roundness. There is no obvious visual indication of spiral arms or a prominent disk structure. The galaxy's central region displays a noticeable concentration of light, potentially indicating a bulge or nucleus. The overall color profile appears relatively red, suggesting an older stellar population with diminished levels of ongoing star formation. No significant merger activity or major disturbances are immediately evident in the galaxy's structure. A small nearby object might be a possible companion galaxy.
