The galaxy presents an overall elliptical morphology, although there are some features that indicate a possible disk galaxy. The central region exhibits a bright, concentrated bulge, appearing somewhat smooth in texture. Proceeding outward, the luminosity decreases, revealing a faint, diffuse halo surrounding the main body of the galaxy. The color is predominantly yellow-orange, suggesting an older stellar population within the bulge. Subtle hints of bluer regions are visible in the outer disk, indicative of ongoing, but low levels, star formation.

There is an asymmetry visible in the galaxy's outer regions. Irregularities hint at a potential interaction or minor disturbance, though no obvious signs of a major merger are immediately apparent. The overall shape can be described as intermediate between a perfectly round form and a cigar shape, with the galaxy appearing elongated.
