The galaxy presents a seemingly smooth morphology with a slight ellipticity. The central region appears relatively bright and concentrated, with an overall yellowish hue. This suggests a population of older stars dominating the core. Extending outward from the center, the galaxy's luminosity gradually decreases. There's some evidence of a fainter, bluer region located towards the periphery of the galaxy, potentially indicating some level of ongoing star formation, although subdued. The overall structure appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. The galaxy's profile suggests a relatively evolved system, possibly transitioning from a spiral to a more lenticular or elliptical form.
