The galaxy presents as an elongated, disk-shaped structure. Its light profile appears relatively smooth, suggesting a well-mixed stellar population and possibly indicative of an older galaxy. There's a subtle color gradient, with a slightly bluer central region fading to redder hues at the edges. This could suggest ongoing star formation in the center, contrasting with an older stellar population in the outer regions. The galaxy's axis ratio is approximately 0.6, indicating that it is moderately inclined with respect to our line of sight. No distinct spiral arms or other prominent features are readily apparent, although the resolution is limiting. There is some indication of tidal disturbance or minor interaction with another nearby object.
