The galaxy appears to be a relatively compact system, exhibiting a generally smooth morphology. There is a slight elongation or asymmetry present, suggesting a deviation from a perfectly elliptical shape. The color profile indicates a redder hue in the central regions, potentially indicative of an older stellar population or dust obscuration. Fainter, bluer extensions can be observed, possibly signaling areas of more recent star formation or tidal features resulting from interactions. The overall structure suggests a lack of prominent spiral arms, though some subtle distortions are visible, hinting at possible past or ongoing gravitational interactions.
