The galaxy exhibits an overall elliptical morphology, displaying a smooth, concentrated central bulge. The bulge is noticeably brighter and more luminous than the surrounding galactic disc. The disc itself appears elongated with a cigar-shaped projection. There's a subtle color gradient visible, transitioning from a bluer hue in the outer regions of the disc to a slightly redder tone towards the central bulge, suggestive of older stellar populations concentrated in the core. Although the overall structure is relatively undisturbed, there's a subtle hint of some minor asymmetry or disturbance, possibly indicating a past or ongoing interaction. No distinct spiral arms are discernible. The galaxy is moderately sized and has a moderate star formation rate.
