The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light distribution appears centrally peaked, indicative of a prominent bulge component. It exhibits an overall elliptical shape, with the ratio of minor to major axis suggesting moderate flattening. There's a faint hint of an extended halo or envelope surrounding the main body. Based on color, the galaxy appears to be comprised of aging stars with very little star formation taking place. There is no clear evidence of spiral arms or prominent dust lanes. There are no indications of any ongoing major merger events, and the overall structure appears relatively undisturbed, with no tidal tails or significant asymmetries.
