The galaxy presents as a relatively smooth structure with a slightly elongated morphology, but is not quite cigar shaped. The central region exhibits a brighter, more concentrated luminosity profile. Some subtle hints of disturbance or features can be seen in the light distribution of this galaxy.

The galaxy shows color variation. The core is bluer, which may indicate ongoing star formation, while the outer regions appear redder, suggesting an older stellar population. The overall color profile suggests a transition in star formation history.