The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. A bright nucleus is apparent, surrounded by a less luminous, diffuse halo of light that diminishes gradually with radial distance. The galaxy exhibits a subtle blue hue, suggestive of a moderate population of relatively young, hot stars, but it could also be affected by redshift. There is no obvious spiral arm structure or dust lane presence. The object appears generally round in shape, lacking a pronounced elongated or distorted appearance. There are no indications of significant ongoing mergers or tidal disturbances.
