The galaxy presents as a somewhat elongated, disk-like structure with a central bulge. The color profile suggests a relatively older stellar population, especially within the bulge region, which appears more yellow-red. There may be some active star formation taking place in a region offset from the main body of the galaxy, with an area presenting with bluer tones. The overall morphology is suggestive of a spiral galaxy viewed at an angle. There is no apparent spiral structure visible, though this could be due to the viewing angle or internal dust obscuration.
