The galaxy presents as a moderately elliptical structure. A central bulge is discernible but not highly pronounced, with the overall light distribution appearing somewhat diffuse. The colour profile suggests a relatively quiescent stellar population, with a blue hue, possibly indicating ongoing, but not excessive, star formation, or possibly just a relatively old stellar population. There is a slight suggestion of a disk component, but without a spiral structure. The shape is slightly distorted, possibly due to an interaction.
