The galaxy exhibits a moderately elliptical morphology, appearing mostly smooth with a high degree of central concentration. The light distribution suggests a significant spheroidal component. A subtle disk-like structure may be present, based on the slight flattening observed. The galaxy displays a color gradient, transitioning from a more yellow/white central region to slightly redder outer regions. This could indicate differing stellar populations, with older, redder stars dominating the outskirts and younger, hotter stars in the central region. There is no obvious indication of a major ongoing merger or strong tidal disturbances, although some minor irregularities cannot be ruled out at this resolution. The galaxy appears relatively isolated. Star formation appears to be suppressed.
