The galaxy presents as a centrally concentrated object with a bright, relatively smooth core. Its morphology appears to be largely spheroidal, with a general absence of distinct spiral arms or a well-defined disk structure. The light distribution suggests a gradual falloff in intensity from the core, indicating a diffuse halo or envelope surrounding the central region. There is faint hint of a disk, maybe at a slight angle to our view. Color variations are subtle, with a tendency toward redder hues, possibly indicating an older stellar population or dust absorption. There is a potential interaction or tidal disturbance suggested by the very slight asymmetries in the outer regions of the galaxy. The galaxy does not appear to be undergoing a major merger, though a minor disturbance cannot be ruled out. The overall impression is that of a galaxy with a mass in the high range with a comparatively small range of star formation.
