This galaxy presents as a somewhat elliptical or lenticular-shaped system, with a bright, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component. The disk does not appear to be strongly structured, lacking prominent spiral arms or dust lanes discernable within the image's resolution. The overall color of the disk appears bluer than the bulge, hinting at more recent star formation activity, though not to an overwhelming extent. The galaxy appears relatively isolated, showing no obvious signs of major tidal disturbances or interactions with nearby galaxies, although there might be some minor asymmetric disturbances. The galaxy appears to be in an intermediate state between a spiral and elliptical, possibly a lenticular galaxy undergoing a slow decline in star formation. The galaxy is not perfectly circular, but in-between circular and cigar-shaped.
