The galaxy appears to be a relatively compact system, exhibiting a generally elliptical morphology. There's a central bright region which likely corresponds to the galactic nucleus. The overall color profile suggests the presence of both older stellar populations which have a redder hue, along with regions of bluer light that may indicate ongoing or recent star formation. Faint disk features or spiral arms might be present but hard to discern. There seems to be some irregular disturbance or tidal features to the south, potentially indicating a minor gravitational interaction with another galaxy or an internal disruption.
