The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its color profile suggests a relatively old stellar population, exhibiting a slightly redder hue in comparison to galaxies with ongoing active star formation. There is no distinct spiral arm structure or prominent dust lanes visible. The galaxy has a relatively compact size, with a diffuse, extended halo of fainter light surrounding the brighter central region. There is little evidence of morphological disturbances such as tidal tails or asymmetries which suggests that there has not been recent major merger activity, although there is some indication of minor disturbance.
