This galaxy presents an elliptical morphology, with a dominant smooth structure. The light distribution is centrally concentrated with a yellowish hue in the core, suggesting an older stellar population. The galaxy appears elongated, exhibiting a cigar-like shape. There is a subtle indication of a disk-like feature, but it is not clearly defined. No significant disturbances or signs of a major merger are visible. The lack of distinct spiral arms or prominent dust lanes further supports the classification as an elliptical galaxy. The outer regions of the galaxy show a fading in intensity, characteristic of a spheroidal distribution of stars.
