The galaxy presents as a relatively compact and concentrated object, exhibiting an overall smooth morphology. The central region is brighter and more condensed, suggestive of a significant bulge component or a high concentration of stars and dust. The surrounding region appears less structured, possibly indicating a faint disk component. The galaxy shows a slight blue hue, particularly towards the central regions, which could indicate ongoing or recent star formation. There's a lack of any obvious spiral arm structure. It's estimated to be of intermediate mass.
