The galaxy presents a relatively smooth, elliptical morphology. The primary body exhibits a concentrated, bright central region, likely the galactic nucleus. There is an absence of prominent spiral arms or well-defined disk structures. The color profile suggests an older stellar population, primarily yellow, with subtle hints of redder areas possibly indicating regions of dust or older, redder stars. Some distortion is present in the lower section, suggesting a possible disturbance or interaction. It appears to be merging with another object, or experiencing a tidal disturbance.
