The galaxy appears as a moderately bright, elliptical-shaped object. Its light is concentrated towards the center, with a smooth, gradual decline in brightness outwards. The color profile suggests a predominantly older stellar population, with light skewed toward the redder end of the spectrum. However, bluer regions may indicate ongoing or recent star formation. No distinct spiral arm structures or prominent dust lanes are visible. There is a slight asymmetry, with one side appearing slightly more extended or disturbed than the other, although a major disturbance is unlikely. The galaxy exhibits a relatively high degree of central concentration, suggesting it is in a more advanced stage of morphological evolution. It is not perfectly spherical, showing an elongated, cigar-like shape. Overall, the galaxy presents the characteristics of a relatively evolved galaxy with a mix of stellar populations.
