The galaxy presents a generally smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. There is a concentrated central bulge, potentially indicative of an older stellar population, from which the luminosity decreases gradually outwards. The color gradient suggests a central region that is whiter and bluer, transitioning to a redder, yellowish hue in the outer regions.

The overall structure exhibits a degree of roundness, appearing neither highly elongated nor perfectly spherical, leaning toward an intermediate shape. There is no distinct evidence of ongoing major merging activity or significant tidal disturbances; the galaxy appears relatively undisturbed. However, there is some irregular light distribution that could be related to minor merger activity. Based on the color profile, some star formation is probably occurring within the galaxy.
