The galaxy appears to be a relatively smooth, elliptical galaxy, displaying a generally rounded morphology. The central region exhibits a high concentration of light, appearing bright and yellowish-white. The light fades gradually as it extends outwards, indicating a decreasing stellar density.  The galaxy lacks any obvious spiral arm structures or strong dust lanes.  There is no evidence of a major merger event, although faint disturbances are possible in the outer regions. The galaxy appears to be a fairly relaxed system, exhibiting characteristics consistent with a quiescent, passively evolving population. Its size is moderate for an elliptical galaxy, indicating a substantial, but not overly massive, stellar component. The overall color suggests a population of older stars, contributing to the yellow-red appearance.
