The galaxy presents a moderately elliptical morphology, appearing neither perfectly spherical nor highly elongated. A central bulge is clearly discernible, exhibiting a concentrated luminosity. There's a noticeable transition from the bright, yellowish core to the surrounding disk. The disk structure itself demonstrates a relatively smooth texture, with limited evidence of prominent spiral arms or significant dust lanes. The color profile suggests a mixture of stellar populations, with the yellower hue of the central bulge potentially indicating a population of older, evolved stars, while the outer regions exhibit a slightly bluer tint, suggestive of ongoing or recent star formation. No obvious signs of a major merger event are apparent, although minor distortions or faint tidal features cannot be entirely ruled out based on this image alone. Overall, the galaxy appears to be a substantial system with moderate star formation activity.
