The galaxy presents as a relatively smooth, elongated structure with a somewhat elliptical morphology. The central region exhibits a higher concentration of luminosity, gradually decreasing towards the outer edges. There appears to be minimal indication of distinct spiral arms or significant star-forming regions upon visual inspection. The overall color profile appears to be more consistent with older stellar populations, exhibiting slightly redder hues. There is a slight indication of distortion in the overall shape which may be evidence of tidal interactions, possibly a minor merger or disturbance. Based on its shape and color, the galaxy may belong to the elliptical or lenticular class, possessing a low rate of star formation and a generally older stellar population.
