The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. The core presents a bright, yellowish hue, suggestive of an older stellar population. There is a lack of distinct spiral arm structure or prominent dust lanes. The galaxy appears mostly spheroidal in shape. There is a subtle color gradient visible, the outer regions display bluer hues, suggesting the presence of some younger stars in the periphery. There's no indication of major merger activity. Slight asymmetry in the galaxy's outer regions may suggest a minor interaction or disturbance.
