The galaxy exhibits a morphology consistent with an early-type, likely elliptical, classification. It presents a generally smooth and rounded appearance with a high central concentration of light. A slight hint of blueness can be observed, but is subtle, and doesn't indicate a strong recent burst of star formation. The galaxy shows no strong evidence of spiral arms, bars, or significant disk structures, but instead presents a near-spheroidal shape. There are no obvious signs of tidal disturbances or ongoing mergers, although a slight asymmetry can be observed. There may be minor interaction with a neighboring galaxy, but it is unresolved. The light profile suggests a relatively smooth and well-mixed stellar population. 
