The galaxy presents an overall smooth morphology with a slightly elongated shape. The light distribution appears concentrated towards the center, suggesting a prominent galactic bulge. There is a subtle color gradient across the galaxy; the core exhibits a distinct bluish-white hue, potentially indicating the presence of younger stellar populations or ongoing star formation, while the outer regions display a slightly redder tone, possibly indicative of older stellar populations. The galaxy does not show any prominent spiral arm structures or distinct dust lanes based on what is visible. The edges of the galaxy gradually fade into the background, with no sharp boundaries detected. No signs of ongoing or recent major merger activity are readily apparent, but the possibility of minor interactions cannot be completely ruled out based solely on visual inspection.
