The galaxy presents an elliptical morphology, with a smooth light distribution, although some disturbance can be observed. The central region exhibits a concentrated, brighter, yellowish-white hue, suggesting an older stellar population likely dominating the core. Moving outwards from the center, the light fades into a less concentrated halo. There's a suggestion of asymmetry or tidal features; possibly evidence of past gravitational interaction or a minor disturbance within the galaxy. The galaxy appears moderately inclined relative to our line of sight. Overall it appears to be a relatively massive system, with low star formation.
