The galaxy appears to be a relatively compact, elliptical system. Its light profile is smooth and centrally concentrated, with a gradual falloff in intensity from the core. The central region exhibits a yellowish hue, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are visible, further supporting the elliptical classification. There is a slight elongation, indicating that the galaxy isn't perfectly spherical. There is no evidence of ongoing major mergers or strong tidal distortions. The overall faint blue emission is not very present, pointing to a low star formation rate.
