The galaxy presents as a relatively smooth, rounded object. It appears to have a concentrated central bulge, exhibiting a yellowish hue, likely indicating an older stellar population within the core. Extending outwards from the bulge is a fainter, more diffuse disc. This disc shows a bluer colouration compared to the central region, implying the presence of younger, hotter stars and potentially ongoing star formation activity, although this is not obviously evident within the image. The overall structure suggests a late-type spiral or lenticular galaxy, with the smooth appearance possibly indicating it is approaching the elliptical end of the morphological sequence. There is no obvious evidence of ongoing major mergers or tidal disturbances.
