The galaxy presents as a roughly elliptical structure, exhibiting a smooth, concentrated central bulge. The bulge displays a yellowish hue, suggesting an older stellar population dominated by redder stars. Surrounding the bulge is a fainter, more diffuse disk component. This disk exhibits a greenish-blue tint, potentially indicative of ongoing star formation and the presence of younger, hotter stars. The galaxy appears relatively undisturbed, with no obvious signs of a major merger or significant tidal interactions. There may be a slight asymmetry in the outer regions of the disk, but this could also be due to image artifacts. Overall, the galaxy seems to be an intermediate-mass system with a mix of old and young stellar populations and no clear spiral structure.
