The galaxy presents as a moderately sized, somewhat elliptical structure. Its light is concentrated towards the center, displaying a bulge-like feature with a yellow-red hue, indicative of an older stellar population. Surrounding the central bulge is a fainter, more diffuse halo, suggesting a relatively smooth overall light distribution. There is a slight flattening or elongation to the structure. No distinct spiral arm features or strong dust lanes are readily apparent. The galaxy appears relatively isolated, showing no obvious signs of major interaction with other galaxies, although there is some evidence of minor disturbances to its form. 
