The galaxy presents as a moderately compact structure. It appears relatively smooth with a slightly elliptical morphology, suggesting a later-type spiral or possibly an elliptical classification. The color profile is centrally concentrated with a subtle yellow-orange hue, potentially indicating a relatively older stellar population, and suppressed star formation. There is no obvious dust lane or spiral arm structure visible at this resolution, lending additional support to an elliptical or lenticular classification. Marginal asymmetric disturbances might indicate a possible minor merger event in the relatively recent past.
