The galaxy presents as a lenticular, cigar-shaped system, generally smooth in appearance with a slight central bulge, and an estimated effective radius of approximately 4.7 kpc. The dominant light appears to emanate from older stellar populations, indicated by the redder hue of the central region. Fainter, bluer light extends along the disk, suggesting some presence of ongoing star formation. However, star formation is likely occurring at a low rate. There is no evidence of significant tidal disturbance or major mergers, although minor interactions cannot be ruled out, as slight disturbances appear on the edges of the galaxy. The galaxy is relatively massive, on the order of 10^9 to 10^10 solar masses. The galaxy is observed to be receding at approximately 10% of the speed of light.
