The galaxy appears as a centrally concentrated object with a relatively smooth, diffuse morphology. There is a central bulge that dominates the light profile, exhibiting a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outwards from the central region, hinting at some ongoing star formation in the outer regions. There are no discernible spiral arm structures visible, but there is a slight asymmetry or minor disturbance visible in the upper region of the galaxy, which may be a minor interaction or tidal feature. The galaxy has an approximately round shape. Overall, the galaxy presents as a relatively massive system with a mix of old and more recently formed stars, possibly undergoing some minor interaction.
