The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a concentrated, yellowish hue, suggesting an older stellar population dominating the central regions. The outer regions display a subtle gradient towards redder tones, which is also indicative of older stellar populations. The galaxy's morphology is elongated, appearing cigar-shaped rather than perfectly spherical. There's no immediately apparent evidence of significant disk structure or ongoing major merging activity, though a possible minor asymmetry could suggest past interactions or minor disturbances. Overall, the galaxy appears to be a mature, relatively quiescent system with a moderately high stellar mass.
