The galaxy presents as a generally smooth, elliptical structure. Its core exhibits a bright, concentrated luminosity, indicating a significant density of stars and potentially the presence of an active galactic nucleus. The galaxy's color profile appears yellowish-white, suggesting an older stellar population with a lower rate of ongoing star formation. The overall morphology suggests a classification towards the early-type end of the Hubble sequence, likely an elliptical galaxy. There is little evidence of spiral arms or significant dust lanes. A slight elongation is perceptible, though the galaxy is mostly rounded. The light distribution decreases gradually from the center outwards, indicating a lack of intense star-forming regions in the outskirts. No obvious signs of recent or ongoing merger events are apparent, as the galaxy appears undisturbed.
