The galaxy appears as a relatively compact, elliptical structure. The core exhibits a higher surface brightness, suggestive of a concentrated stellar population and/or an active galactic nucleus, though no distinct jet is visible. The isophotes appear generally smooth and regular, indicating a well-relaxed system without prominent tidal features or signs of recent major mergers. A slight color gradient is observed, with the central regions exhibiting a more yellow/white hue, potentially indicating an older stellar population in the bulge, while the outer regions show a faint reddish tint, which could indicate the presence of dust or a slightly younger, cooler stellar population. No distinct spiral arm structure or dust lanes are apparent. The galaxy’s overall morphology is consistent with an early-type galaxy, likely an elliptical galaxy with an approximate mass range of 10^10 M☉. The star formation rate appears low, given the lack of prominent blue regions that are commonly observed in actively star-forming galaxies.
