The galaxy presents as a predominantly smooth structure, exhibiting a high degree of central concentration. Its overall shape approximates a circular morphology, deviating slightly towards an elliptical form. There is a subtle suggestion of a disk component, though this is not sharply defined. The color profile indicates a population of older stars, particularly concentrated in the bulge region, which appears more yellow. Fainter blue star forming regions are visible in the disc, showing its spiral arm structure is very faint, but detectable. No obvious tidal features or major disturbances indicative of ongoing merger activity are apparent, although there seems to be a faint disturbance in the center of the galaxy, suggesting there has been a minor merging event in its past. The galaxy's texture appears relatively uniform across its surface, implying a lack of prominent dust lanes.
