The galaxy exhibits a predominantly smooth morphology. It appears as a single, relatively consolidated light source, lacking prominent spiral arms or a well-defined disk structure. The overall shape appears to be mildly elliptical. There appears to be some minor disruption. The core presents a concentrated area. There may be a faint indication of tidal tails or other faint stellar streams that may indicate interactions with smaller galaxies. The color profile suggests a relatively evolved stellar population.
