The galaxy appears as a centrally concentrated, luminous object. Its overall morphology suggests a largely smooth structure, with a predominantly elliptical shape. The light distribution appears relatively uniform and lacks any prominent spiral arm features or distinct dust lanes. There is a slight elongation, hinting that it is not perfectly spherical. The core exhibits a yellowish or orange hue, possibly indicative of an older stellar population. Fainter, bluer light is present around the central region, indicating more recent star formation at a lower rate. There are no signs of any major mergers or significant tidal disturbances, suggesting this is an isolated galaxy, not undergoing major interactions. The overall impression is of a mature galaxy with characteristics of an early-type system.
