The galaxy presents a primarily smooth morphology, with a centrally concentrated light profile. The shape is neither perfectly round nor highly elongated, appearing somewhere in between. The core of the galaxy exhibits a brighter, more luminous region, suggesting a higher density of stars or perhaps an active galactic nucleus. A subtle blueish tint is observable throughout the galaxy, indicating the presence of some younger stellar populations, though overall the galaxy does not show prominent features indicative of ongoing, intense star formation. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity, however, a slight asymmetry might suggest a minor interaction or disturbance. The overall impression is that of a relatively evolved system, likely with a substantial stellar mass.
