The galaxy in question appears as a moderately luminous object with an elliptical morphology. It presents a reddish hue, suggestive of an older stellar population with ongoing, but relatively low, star formation activity. There is evidence of a generally smooth profile, but also subtle features that might indicate minor disturbances or asymmetries in its structure. The overall shape is elongated, leaning towards a cigar-like appearance rather than perfectly round. There is no prominent central bulge or disk structure easily discernable in the image. There is no visually obvious sign of major merging or strong tidal interactions.
