The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, displaying a yellowish hue, indicative of an older stellar population. Moving outward from the core, the galaxy transitions to a bluer color, suggesting the presence of younger, hotter stars. The overall shape is elongated, approaching a cigar-like form, with a suggestion of minor disturbances within its structure, possibly from a past interaction. Star formation appears to be ongoing, as evidenced by the blue regions. The galaxy does not appear to be undergoing a major merger, but there might be minor disturbances.
