The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. A slight extension of the light profile is visible, indicating a possible disk or some form of extended structure, however, distinct spiral arms are absent. There is a minor red region to the left, indicating an area with dust or a young stellar population that stands out due to its color, suggesting a possible minor disturbance or ongoing localized star formation. The overall roundness suggests a possible elliptical or lenticular classification. The lack of significant distortions in the main body implies that the galaxy is not currently undergoing a major merger event, though the minor red feature could point towards a very subtle interaction.
