The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The galaxy exhibits a radial color gradient, transitioning from a bluer periphery to a redder core. This color variation suggests a potential difference in stellar populations and star formation activity, with older, redder stars dominating the core and younger, bluer stars residing in the outer regions. There is subtle evidence of possible tidal disturbances or minor interactions, potentially influencing the galaxy's morphology, especially in the distribution of its outer stellar halo. These asymmetries could be indicative of past or ongoing accretion events or gravitational interactions with smaller companion galaxies. There's a possibility of minor dust lanes or features, which would require higher resolution to confirm, and suggest recent or ongoing low levels of star formation.
