The galaxy presents a predominantly smooth morphology, exhibiting a high degree of central concentration. Its shape is generally round, with only a slight deviation from perfect circularity. There is no discernible spiral arm structure or prominent disk component visible. The color profile suggests a relatively older stellar population, with a yellowish hue dominating the central region. There is no indication of any major ongoing merger activity or significant tidal disturbances. Faint and diffuse light extends outwards from the core of the galaxy, indicating a relatively large effective radius. There is no strong evidence of active star formation regions within the observable portion of this galaxy.
