The galaxy appears to be a relatively smooth, elongated system, likely an elliptical or lenticular type. Its color profile suggests a population of older stars, indicated by the reddish hue near the central bulge. There is a subtle gradient from a brighter, yellower core region outwards to fainter, bluer edges. The galaxy's shape is noticeably cigar-shaped, exhibiting a clear departure from perfect circularity. No distinct spiral arms or dust lanes are visible. The overall structure suggests a gravitationally relaxed system, showing evidence for a minor tidal disturbance in its form. The rate of new star formation is not significant. 
