The galaxy presents as a generally smooth, elliptical object with a moderate degree of flattening. The central region exhibits a brighter, more concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus. The color gradient appears relatively uniform across the galaxy, with a yellowish hue indicating an older stellar population. There is no apparent evidence of spiral arm structure or significant dust lanes. Faint extensions or tidal features are not readily discernible, suggesting a relatively quiescent state in terms of recent mergers or interactions. The morphology suggests a classification as an elliptical galaxy, likely with a substantial mass and relatively low star formation rate.
