The galaxy presents as a relatively smooth, elliptical-like structure. There is a noticeable concentration of light toward the central region, suggesting a prominent galactic bulge. The overall color appears yellowish-orange, hinting at an older stellar population within the galaxy. No distinct spiral arms or significant dust lanes are apparent. The morphology suggests this galaxy is likely an elliptical or S0 type, with minimal signs of ongoing star formation. The isophotes are somewhat elongated, but not significantly cigar-shaped, indicating a moderate degree of ellipticity. There is no visible evidence of tidal tails, disrupted morphology, or obvious merging activity. The smooth appearance suggests a gravitationally relaxed system, likely the result of past mergers that have since settled.
