The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile. It appears elongated, with a cigar-like shape. There is no evident spiral arm structure or dust lane obscuration. The central region exhibits a yellowish-white hue, potentially indicating a population of older stars. Fainter, bluish regions can be observed around the periphery. The galaxy's morphology suggests a relatively quiescent system, lacking significant recent star formation activity. There is no clear evidence of interactions or major mergers in its recent past. Overall, the galaxy appears as a mature system with a predominantly smooth stellar distribution.
