This galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and featureless morphology. There is no discernable disk or spiral arm structure. The light profile suggests a concentration towards the center, with a radial decrease in luminosity. The galaxy is slightly round. There are no signs of recent major merger activity or significant tidal disturbances, though minor disturbances cannot be ruled out. The color profile shows a dominance of redder hues, indicating an older stellar population. There is no significant presence of dust lanes or prominent star-forming regions. The estimated effective radius is approximately 1.26 kpc. The object’s star formation rate is generally low. Its mass is roughly within the range of dwarf galaxies.
