The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a high stellar density. Moving outward from the core, the luminosity gradually decreases. There's a slight elongation, a cigar-shaped structure in its overall form, but the light distribution remains fairly uniform, without distinct spiral arms or prominent dust lanes visible. The color appears to be a relatively red-shifted hue, suggesting an older stellar population and potentially lower current star formation activity. The galaxy appears to be isolated, exhibiting no signs of major ongoing merger activity or significant tidal disturbances, though there may be a minor disturbance present. 
