The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth morphology with a centrally concentrated bulge. The color profile suggests a mix of stellar populations, with the core region showing a yellower, possibly older stellar population. Fainter blue light is diffused towards the edges of the disk, indicating ongoing or recent star formation. There is no evidence of strong spiral arm structure or prominent dust lanes. The galaxy is relatively isolated, showing a lack of significant tidal disturbances or interactions with nearby galaxies, although there is the slightest distortion to one side of the galaxy.
