The observed galaxy presents as a relatively compact, yet somewhat amorphous, structure. Its overall color profile appears to be dominated by light from older stellar populations, exhibiting a yellowish to reddish hue. There is a slight asymmetry in the distribution of light within the galaxy, indicating a potential disturbance. Faint wisps or tails are possibly visible, extending from the main body of the galaxy. These features suggest a minor interaction or tidal disruption event. While the bulk of the galaxy's luminosity is concentrated in a central region, there's little evidence of prominent spiral arms or a well-defined disk structure. Overall, the galaxy appears to be relatively smooth. A subtle disruption is seen, hinting at a past or ongoing interaction with another galaxy.
