The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. Its color profile appears consistent, trending towards redder hues, particularly in the core region. There is no discernible spiral structure, prominent dust lanes, or evidence of ongoing major mergers in this image. Minor distortions are not apparent, suggesting a relatively relaxed structure. The general appearance points towards a galaxy with a significant spheroidal component and a moderate mass. The redder color and absence of prominent star-forming regions suggest a low specific star formation rate.
