This galaxy exhibits a generally smooth morphology, with a likely flattened spheroid shape. The light distribution appears concentrated towards the central region. Based on observed morphology, a possible estimation of the size puts the galaxy at approximately 5.6 kpc across. There is some suggestion of disturbance to the main body, possibly the result of minor interactions or tidal effects, which may explain the elongated shape. The galaxy's color suggests it is not exclusively comprised of old stars. Overall, this galaxy likely exhibits ongoing but relatively low levels of star formation activity. There is a relatively high probability that this is a galaxy involved in an ongoing merger.
