The galaxy presents as a somewhat asymmetrical system. The central bulge exhibits a yellowish-white hue, suggesting a population of older stars. Extending outwards, a fainter disk is visible. There is some evidence of spiral structure, although it appears rather indistinct and ill-defined. The color of the disk graduates towards a bluer tone, indicative of ongoing star formation. There is no clear sign of any major disturbances or strong tidal features which may indicate a recent merger. The galaxy appears relatively isolated with no strong evidence of any nearby interacting galaxies or tidal distortions. Overall, this appears to be a relatively undisturbed spiral galaxy with moderate star formation occurring in its disk region.
