The galaxy presents an overall elliptical morphology with a moderately high degree of smoothness. There is a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The outer regions appear more diffuse, with a subtle bluish tint indicative of some younger, hotter stars, though star formation appears to be relatively low. There's a slight deviation from perfect roundness, leaning towards a more oblate spheroid shape. No clear spiral arm structure or bar is discernible. There's a hint of a minor disturbance or asymmetry in the outer envelope on the left side, possibly indicating a past or ongoing minor interaction. The galaxy does not appear to be a major merger system.
