The galaxy presents an elongated, cigar-shaped morphology. It displays a relatively smooth light distribution with a concentrated central region. The color profile suggests a predominantly older stellar population, with a redder hue dominating the galaxy's core. There are hints of bluer regions at the edges, potentially indicating areas of ongoing or recent star formation, though it is quite subdued. The galaxy does not appear to show any strong signs of spiral arm structure or significant disturbances, such as tidal tails or obvious merger signatures. The overall impression is that of an evolved, possibly quiescent system.
