The galaxy presents a centrally concentrated morphology, with a bright, yellowish core indicative of an older stellar population. Surrounding the core is a fainter, more diffuse halo exhibiting subtle bluish tinges, suggesting the presence of some younger stars or ongoing star formation regions. The overall shape appears somewhat irregular, potentially indicative of past or ongoing interactions. There might be some signs of minor tidal disturbances in the outer regions. No distinct spiral arm structure is discernible.
