The galaxy presents a generally smooth morphology, displaying an elongated, cigar-shaped profile. The dominant colour is yellowish-white, but with hints of a bluer hue towards one edge and some subtle redder tones towards the other. The bluer region indicates the presence of a moderate amount of younger, hotter stars in the area. Conversely, the redder region may suggest a higher concentration of older stars and dust. There is no clearly defined spiral structure visible, nor are there any strong indications of a recent major merger event, though a minor tidal interaction cannot be ruled out. Overall, the galaxy seems to have a moderate star formation rate, with specific star formation indicative of a quiescent nature. The galaxy is not perfectly symmetrical, and it displays some structural irregularities.

