The galaxy presents as a relatively smooth, elongated structure. Its overall color profile suggests a population dominated by older stars, exhibiting a reddish-yellow hue in the central regions. The core is bright and concentrated. Fainter, bluer regions can be seen, indicating some recent star formation activity. It appears disk-like, but largely featureless, with no obvious spiral arm structures or significant dust lanes visible. The shape is elongated, likely viewed at an oblique angle. There is no indication of any major ongoing merger events, although there is some slight asymmetry, suggesting possible minor gravitational interactions.
