The galaxy presents a generally smooth morphology, with a slightly elongated, cigar-shaped appearance. The light distribution appears centrally concentrated, exhibiting a bright, yellowish core, which could be indicative of an older stellar population. The galaxy does not display prominent spiral arm structures or significant dust lanes. There appears to be some faint blue light on the periphery of the galaxy, which would imply the presence of some star formation. There is only minor apparent disturbance in the system based on this image. The color gradient suggests possible radial changes in stellar populations, but without spectroscopic data, this remains speculative. The estimated size suggests that this is a larger galaxy. Overall, the galaxy appears to be a relatively evolved system.
