The galaxy presents as a smooth, elongated structure. Its overall form is consistent with an elliptical or lenticular morphology, displaying a cigar-like shape. The light distribution appears centrally concentrated, with a gradient towards the outer regions. The core exhibits a yellowish hue, possibly indicative of an older stellar population. Outer regions display bluer tones, which may represent younger star formation. There appears to be minor tidal disturbances nearby, with a possible faint companion visible. No prominent spiral arms or strong dust lanes are apparent. Overall, the galaxy shows evidence of a significant mass and a moderate rate of star formation.
