This galaxy presents as an elliptical morphology. The light distribution is dominated by a smooth, centrally concentrated component, characteristic of an older stellar population. The core appears to be yellowish, suggesting the presence of evolved stars. There's no distinct spiral arm structure or prominent dust lanes visible. The galaxy appears somewhat elongated in shape, exhibiting a cigar-like appearance. No major signs of ongoing mergers or major disturbances can be seen, although some minor irregularities cannot be ruled out due to image resolution. Overall, this galaxy appears to be a relatively undisturbed, early-type system.
