The galaxy presents as a centrally concentrated, relatively smooth object, likely an elliptical galaxy. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light distribution decreases gradually from the center outwards, indicating a relatively high degree of symmetry and little evidence of spiral arms or prominent disk structures. A subtle extension or slight asymmetry is visible along the horizontal axis, possibly indicative of a minor tidal interaction or past merger event. The galaxy is neither perfectly round nor elongated, but something in between. It exhibits a moderate redshift, suggesting it is at an intermediate cosmological distance. Based on color, morphology, and inferred distance, the galaxy is likely a passively evolving system with a relatively low rate of star formation. Overall the galaxy appears to be non-merging. 
