The galaxy presents as a relatively smooth, centrally concentrated object, approximately circular in projection. The light profile indicates a central bulge with a yellowish hue, suggesting an older stellar population. Surrounding the bulge is a more diffuse, bluish-greenish disk component, potentially indicating the presence of some younger stars and ongoing, albeit low, star formation. No distinct spiral arms or bar structures are readily apparent. There are no obvious signs of a major merger or significant tidal disturbances, although subtle asymmetries cannot be ruled out at this resolution. The galaxy appears to be a relatively isolated system.
