The galaxy presents as a well-defined, elongated structure, suggesting an elliptical or lenticular morphology. The central region exhibits a bright, concentrated core, indicative of a high stellar density. The light profile appears relatively smooth with a yellow-gold hue in the central bulge. The disk component, while present, isn’t as prominent, displaying subtle blue tones, perhaps suggesting the presence of some younger stellar populations. There is no distinct evidence of spiral arms. The outer regions show a gradual fading, suggesting a smooth transition into the surrounding space. Faint asymmetry can be detected at one end of the galaxy, which could suggest minor interaction or disturbance. There are no clear indications of strong star-forming regions or recent merger events.
