The galaxy presents as a flattened spheroid, exhibiting a moderate ellipticity. Its color profile appears relatively uniform across the observed bands, with a general red hue, suggesting a dominant population of older stars. There is no strong evidence of spiral arm structures, bars, or significant dust lanes, contributing to a relatively smooth overall appearance. Faint color variations may indicate subtle internal structures, though the resolution limits detailed morphological classification. There's no visual evidence of a current major merger event, though possible minor tidal features are too faint to conclusively establish an ongoing interaction. The galaxy appears as a quiescent system with a low rate of star formation.
