The galaxy presents as a generally smooth, elliptical structure with a concentrated central bulge. It exhibits a yellow-orange hue, suggestive of an older stellar population with fewer ongoing star formation events. The galaxy is largely featureless, lacking prominent spiral arms or dust lanes. There is a slight elongation, appearing closer to round than cigar shaped, suggesting a moderate ellipticity. No major merger activity or tidal disturbances are immediately apparent. There might be very slight disturbance, but likely none or very minor.
