The galaxy presents an elliptical morphology. Its overall appearance is smooth, suggesting it is composed primarily of older stars and has undergone little recent star formation. The galaxy exhibits a slightly elongated shape, resembling a cigar, rather than a perfect sphere. There is no clear evidence of spiral arms or a prominent disk structure. The color distribution appears fairly uniform across the galaxy, with a slight redder hue, indicating an older stellar population. There are no obvious signs of an ongoing merger or major tidal disturbances. The galaxy’s structure indicates that it may be undergoing quiescence.
