The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright, yellowish hue, likely indicating an older stellar population. Moving outwards, the colour gradually shifts towards a bluer, fainter gradient, suggesting a possible presence of some younger stars in the outer regions, although the dominant stellar population appears to be aged. There is no obvious evidence of spiral arms or other disk-like features. The galaxy appears mostly undisturbed, with no distinct signs of recent or ongoing major merger activity, however, there are some minor disturbances in the outer regions. The overall shape is not perfectly spherical, exhibiting a slight elongation, appearing intermediate in roundness, somewhere between perfectly round and cigar-shaped.
