The galaxy presents a morphology consistent with an elliptical galaxy. The light distribution appears smooth and centrally concentrated, with a noticeable elongation suggestive of a cigar shape. There is little evidence of spiral arm structure or significant dust lanes. The core region exhibits a bright, concentrated luminosity. Fainter, bluer light extending from the core indicates some ongoing, low-level star formation. The galaxy appears to be relatively undisturbed, with no signs of major mergers or tidal interactions.
