This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. Its shape appears elongated, but it could be described as mostly in between shapes as it is neither perfectly round nor highly elongated. There is a suggestion of minor disturbances within the galaxy's structure, but these do not dominate its overall appearance, however, given the elongated nature, these could indicate the presence of minor tidal interactions, perhaps from a past merger event. The galaxy shows a radial gradient in color, being considerably bluer at the outer edges than in the central core. The object does not show evidence of significant ongoing star formation.
