The galaxy presents as a likely spiral type, though the resolution limits detailed morphological classification. It appears as a single, somewhat indistinct central bulge that is bright and slightly elongated. Some faint, diffuse emission extends outwards on either side of this core, suggesting a possible disk structure. The galaxy exhibits a color gradient, with the bulge appearing more yellowish in contrast to the slightly bluer hues in the potential disk. There is no evidence of strong spiral arm structure or prominent star-forming regions directly visible in the image. It displays no major disturbance but may present slight signs of tidal interactions.
