The galaxy presents a generally smooth appearance, with a cigar-like, elongated shape. There are no prominent spiral arms or disk structures visible. The light distribution appears relatively uniform, with a slight concentration towards the center. A faint color gradient is observable, shifting from a slightly bluer hue at the edges to a redder hue in the central bulge. This may indicate differences in stellar populations and activity across the galaxy, with older, redder stars more concentrated towards the center and younger, bluer stars possibly residing in the outer regions. There is no indication of major merger activity or significant tidal disturbances. Based on these observations, it appears to be a small elliptical or lenticular galaxy. Star formation rates are suppressed.
