The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-red hue, suggesting a population of older stars and a lack of significant ongoing star formation. There is a small amount of bluer light visible in the galaxy, suggesting some star formation is likely still present, though at a low level. The galaxy appears isolated with no clear evidence of ongoing major mergers or tidal disturbances based on the observed morphology. The light distribution suggests an axially symmetric form with a high degree of central concentration. The object is relatively compact on the sky.
