The galaxy appears to be an elliptical type, exhibiting a generally smooth and centrally concentrated light distribution. It presents an elongated shape, tending towards a cigar-like morphology. A distinct bulge component is visible, dominating the central region with a bright, concentrated luminosity. There is a notable absence of well-defined spiral arms or significant dust lanes. The galaxy's color profile suggests a population of older stars, contributing to the reddish hue. Faint hints of a disk may be present surrounding the bulge. Any signs of a recent or ongoing major merger are not apparent based on the present imagery.
