This galaxy exhibits a prominent, elongated shape, with its longest axis significantly exceeding its shortest. It displays a relatively smooth texture, suggesting a lack of significant spiral arm structure or large, distinct star-forming regions. The galaxy's central region appears more concentrated and exhibits a slightly redder hue, potentially indicating an older stellar population or a higher dust concentration. The outer regions show a bluer tint, possibly indicating the presence of younger stars or a lower concentration of dust. There is no obvious indication of active merging events or major tidal disturbances, although minor disturbances or interactions cannot be ruled out based on the available imagery. Overall, it seems to be a moderately sized galaxy with a relatively quiescent morphology.
