The galaxy presents as a somewhat elliptical structure, appearing neither perfectly spherical nor highly flattened. The light distribution suggests a concentration of older stellar populations in the central region, indicated by a yellowish hue. Moving outward from the core, a subtle transition occurs, showing hints of bluer star formation regions.

While no distinct spiral arms are discernible, the overall texture exhibits a degree of irregularity or possible disturbances. There may be minor disturbances within the galaxy, suggesting tidal interactions.

The galaxy's size is moderate, occupying a noticeable but not dominant portion of the field of view. It exhibits moderate luminosity. The observed morphology is generally consistent with a system undergoing some level of internal evolution or external influence, without signs of a major merger event.
