The galaxy presents as a single, diffuse object with a generally smooth morphology. Its overall shape appears elliptical, elongated slightly along one axis. The light distribution is concentrated towards the center, exhibiting a bright core. The color is predominantly redder, suggesting an older stellar population or significant dust content. There is minimal evidence of spiral arms, distinct star-forming regions, or irregular features within the visible structure. Possible minor tidal disturbance of the galaxy itself. The galaxy appears relatively isolated. 
