The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its morphology is characterized by a centrally concentrated light profile that fades gradually towards the outer edges. While there is no prominent spiral structure evident, a subtle disk-like feature might be present within the fainter, outer regions. There appears to be a lack of significant dust lanes or prominent star-forming regions within the visible portion of the galaxy. The galaxy presents a moderate degree of ellipticity, leaning toward a slightly elongated shape rather than being perfectly spherical. There is a possible indication of minor gravitational disturbance or interaction with a neighboring galaxy in the form of a slight asymmetry or distortion in the outer halo. Overall, the galaxy appears to be a relatively evolved system with a relatively low rate of ongoing star formation.
