The galaxy presents a relatively smooth, centralized structure, hinting at an elliptical or lenticular morphology. There's a pronounced central bulge, appearing brighter and more condensed than the surrounding regions. A slight flattening suggests it isn't perfectly spherical. The color profile indicates a somewhat evolved stellar population. The overall blue hue suggests recent star formation, though the presence of redder tones toward the outer edges implies a mix of stellar ages, with older, redder stars possibly populating the outskirts. There are some subtle disturbances evident in the galaxy's morphology, possibly indicators of a minor merger or tidal interactions with a neighboring galaxy. There is no clear evidence of spiral arms or a prominent disk structure.
