The galaxy presents as a cigar-shaped, smooth object, exhibiting an elongated morphology. There's a notable central concentration of light, likely indicating a bulge. The galaxy's color gradient suggests a stellar population that is relatively old and not actively forming many stars. We observe no obvious signs of spiral arms, bars, or prominent dust lanes; the overall structure appears fairly uniform and undisturbed. The object displays a color profile tending toward the redder end of the spectrum. A minor disturbance might be present, but is difficult to confirm from this image. The galaxy appears to be a relatively isolated system.
