The galaxy presents as a relatively small, somewhat diffuse object. The overall morphology suggests a structure that is neither distinctly spiral nor elliptical, possibly lenticular or irregular. There appears to be a dominant central bulge which is bright and has a blue hue, which suggests ongoing star formation. Around the central bulge, there is some irregular and diffuse nebulosity extending outward, with a redder color suggesting older stellar populations or dust extinction. The asymmetry suggests a possible recent or ongoing interaction with another galaxy, but no distinct tidal features are obviously visible in the image. Overall, the galaxy exhibits a blended morphology with a central concentration of stellar activity and surrounding less distinct stellar regions.
