The galaxy presents as a cigar-shaped, relatively smooth, and featureless structure. Its core appears as a concentrated region of light, fading into a gradual halo of diffuse light. This suggests an elliptical morphology, with a possible evolved stellar population dominating the emission. While the main body appears smooth, there are subtle hints of underlying structures, with faint, irregular features. These could potentially indicate minor disturbances within the galaxy. No evidence of a major ongoing merger or strong tidal interactions is apparent. The galaxy appears fairly isolated, and the dominant color is blue, suggesting the presence of cooler stars.
