The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. Its color gradient suggests a dominant older stellar population, contributing to its overall yellowish-orange hue. There appears to be minimal evidence of spiral arms or significant dust lanes. The galaxy exhibits a relatively symmetrical shape, with a slight deviation from a perfect circle suggesting a degree of elongation or possible tidal interaction, although this requires further investigation. The overall appearance is consistent with a passively evolving galaxy, possibly at a redshift of approximately 0.32, given its apparent size and brightness.
