The object presents as a relatively compact galaxy, exhibiting an overall elliptical morphology. The galaxy appears elongated, with a significantly higher aspect ratio, more akin to a cigar shape. Its light profile suggests a relatively smooth distribution of stellar populations, although the presence of some internal structure, potentially suggestive of a disk component or faint spiral arms, cannot be entirely ruled out due to the image resolution. The color is notably redder, implying an older stellar population and potentially lower levels of on-going star formation within the galaxy. A smaller, rounder object, possibly a satellite galaxy or a background source, is visible in close proximity to the main galaxy, but does not appear to be heavily interacting. There are no strong indications of major mergers or tidal disturbances evident in the image.
