The galaxy presents a generally smooth, elliptical morphology. Its central bulge is prominent and appears relatively spherical, exhibiting a concentrated, yellowish color profile suggestive of an older stellar population. There is minimal indication of spiral arm structure or a defined disk. Faint reddish patches are observed within the galaxy, possibly indicating regions of on-going or recent star formation. The overall light distribution suggests that the system is dominated by older stars, with a low rate of star formation. The galaxy's shape does not show any strong signs of tidal disturbances or interactions with other galaxies, indicating that it may be a relatively isolated system or that any past interactions were minor.
