The galaxy presents as a moderately luminous object with an elliptical morphology. Its core exhibits a bright, concentrated region indicating a high stellar density. The galaxy appears relatively smooth, with no distinct spiral arms or prominent dust lanes visible at this resolution. There's a slight elongation to its overall shape but it's not exceedingly cigar shaped. There is some visual evidence of a possible minor interaction or disturbance given the slight asymmetry observed in the outer regions but not an extreme merger. The color profile suggests a population of older stars, giving it a reddish-yellow hue. Overall, this galaxy appears to be a relatively massive, passively evolving system at an appreciable distance, as evidenced by the redshift.
