This galaxy appears to be a spiral galaxy, observed at an angle that is significantly inclined to our line of sight, presenting an elongated profile. The central bulge is prominent and exhibits a smooth, concentrated brightness distribution, suggesting a relatively old stellar population dominating this region. Fainter spiral arms extend outwards from the bulge, showing hints of blue colors. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. However, there is some evidence of minor irregularities within the arms. The light distribution is mostly smooth, but some clumpiness is visible in the arms, which may indicate the presence of regions of ongoing or recent star formation. The galaxy is relatively compact, with the spiral structure confined to a small area around the bulge. The color gradients suggest a redder core with bluer outer regions, typical of spiral galaxies with ongoing star formation in the disk.
