The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be largely elliptical with a high degree of roundness in its overall shape. There is a slight elongation, however, the aspect ratio doesn’t suggest a highly flattened disk system. The galaxy's light distribution indicates a bright core that decreases smoothly outwards, displaying a lack of distinct spiral arm features or prominent dust lanes. There is little evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's overall structure, though minor disturbances cannot be ruled out. Color analysis reveals a general redder hue, which may indicate an older stellar population.
