The galaxy presents as a smooth, elongated, cigar-shaped object. The central region exhibits a higher concentration of light, appearing brighter with a yellowish hue. This suggests an older stellar population is dominant in the core. Progressing outwards from the core, the intensity of light gradually diminishes, and the colour transitions toward a bluer shade. This may be indicative of ongoing star formation within the outer regions of the galaxy. The overall morphology suggests a possible elliptical or lenticular classification with a slight disk, showing possible minor disturbances. There is no readily apparent spiral structure or presence of prominent dust lanes from this vantage point. 
