The galaxy presents an overall elliptical morphology, appearing elongated with a cigar-like shape. The light distribution suggests a smooth profile, indicative of a relatively featureless structure. The central region exhibits a bright, concentrated core that gradually fades towards the outer edges, suggesting a dense stellar population. Color gradients appear subtle, showing a yellowish hue in the core transitioning to slightly bluer tones in the fainter, extended regions. This may suggest ongoing, but limited, star formation in the outer regions compared to the core. There are no prominent spiral arms or obvious signs of significant tidal disturbances or interactions with other galaxies.
