The galaxy appears as a single, relatively smooth object with a concentrated central bulge. The color gradient transitions from a yellowish-white core to a dimmer, reddish outer halo. The smooth and somewhat rounded morphology suggests an elliptical galaxy, or potentially a spiral galaxy viewed from a significant angle where prominent spiral arms are not discernible. There is little evidence of distinct features such as dust lanes or prominent star-forming regions. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major merger activity, though there may be some minor tidal disturbances. The light distribution appears centrally concentrated, indicating a significant concentration of stellar mass in the core. Based on the color and lack of distinct blue regions, it's plausible that the galaxy has a lower rate of current star formation.
