The galaxy presents a generally smooth and rounded morphology, characteristic of an elliptical or S0 type. There is a concentrated central bulge, which displays a yellowish-orange hue. This color suggests a population of older stars. The isophotes are largely regular, showing a high degree of ellipticity. There is little evidence of significant spiral arm structure or ongoing major mergers. However, there appears to be a very faint, subtle disturbance to the smooth profile, perhaps suggesting a minor interaction in the recent past. The galaxy appears relatively isolated.
