The galaxy presents as a somewhat elongated, smooth object with a notable central bulge. The overall color appears bluish, suggesting the presence of relatively young, hot stars. There is no obvious spiral structure or prominent dust lanes visible, which implies that the galaxy is likely an early-type spiral or lenticular galaxy, possibly tending towards an elliptical morphology. The light intensity appears to gradually fade from the center outwards, exhibiting no sharp edges. There might be a very faint, extended halo surrounding the main body of the galaxy but this is difficult to ascertain due to the image's resolution and background noise. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, although a slight asymmetry in its shape could be indicative of a minor interaction in its past.
