The observed galaxy exhibits a smooth, elliptical morphology. It appears largely featureless with no discernible spiral arms or bar structure. The galaxy has a somewhat elongated shape, with a cigar-like appearance.

There's a central concentration of light, suggesting a nucleus or bulge. The color profile transitions from a yellowish hue at the core to a bluer tint towards the outer edges. This color gradient could indicate differing stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars populating the outer regions. There is no obvious sign of tidal tails or other major disturbances, suggesting the galaxy is relatively isolated and not currently undergoing a major merger event, though a minor interaction cannot be ruled out based on this image alone.
