The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology. Its light profile appears to decline gradually from the core, indicating a lack of distinct spiral arms or features. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions transition to a redder color, which may also indicate an older stellar population. The galaxy's overall structure suggests a relatively evolved system, likely an elliptical galaxy. There is no obvious disk structure, and the galaxy seems to be fairly isolated. There is a slight suggestion of a tidal tail or plume on the left side of the object, suggesting it may have merged with another object at one point. No significant dust lanes are discernible.
