The galaxy appears to be a relatively smooth, though slightly elongated, object. It has a moderately concentrated central region that gradually fades outwards with no sharp edges. The overall color profile suggests a somewhat older stellar population, with more light in the redder wavelengths compared to bluer wavelengths. There are some subtle indications of features that could be related to a possible minor disturbance in morphology, but these are not distinct. The lack of strong spiral arm features or prominent star-forming regions is noted, suggesting a quiescent star formation rate. The galaxy exhibits an intermediate level of roundness.
