The galaxy presents as a relatively smooth, elongated structure. Its overall morphology appears to be somewhere between elliptical and disk-like, leaning towards a more ellipsoidal shape. The central region exhibits a notable concentration of light, indicative of a prominent bulge. Moving outward from the center, the light intensity gradually decreases. The color profile suggests a population of older stars, particularly towards the center, with a redder hue, and bluer arms with ongoing star formation. Faint disk structure is visible, but largely washed out by its bulge. There may be a slight indication of tidal disturbance on one side of the galaxy, suggesting a possible past interaction.