The galaxy presents a largely smooth morphology, suggesting it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy exhibits a concentrated central bulge with a gradual fall-off in luminosity outwards. There is little evidence of spiral arms or significant dust lanes. The color appears to be dominated by yellow-red hues, indicative of an older stellar population. The relatively uniform color distribution further supports the classification as an elliptical galaxy, or potentially a lenticular galaxy with a well-mixed stellar population. The galaxy appears to be relatively undisturbed, with no obvious signs of a recent merger or tidal interactions. Overall, this galaxy appears to be a mature system with limited ongoing star formation.
