The galaxy presents as a luminous, elongated structure with a generally smooth appearance, suggesting a relatively evolved system. There is a noticeable central concentration of light, likely a bulge, with a more diffuse surrounding halo or disk. The galaxy displays an overall yellowish hue, possibly indicating an older stellar population and a lower rate of on-going star formation. It is mildly elongated, appearing to be more cigar-shaped than perfectly circular. There is a possible minor disturbance or interaction visible, based on the asymmetry and a slight distortion in the overall shape. This could suggest a past merger or gravitational interaction. The primary light is centrally concentrated and decreases in intensity towards the edges.
