The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration. Its color is predominantly yellowish, suggesting an older stellar population. There is a lack of distinct spiral arm features or prominent dust lanes. The galaxy appears nearly round, with no obvious elongation or distortion. There's no evidence of any major ongoing merger activity or significant tidal disturbances affecting its overall morphology, although there appears to be some subtle irregularities on the edges.
