This galaxy appears to be an elliptical type, exhibiting a generally smooth light distribution with no obvious spiral arms or bar structure. Its shape is elongated, leaning towards a cigar-like appearance. The central bulge is luminous, exhibiting a bright and concentrated core that decreases in intensity towards the outskirts. The color profile indicates a redder hue overall, which suggests a population of older stars and less active star formation. There is a hint of possible interaction or minor disturbance visible in the galaxy's morphology, suggesting a possible ongoing or recent merger event.
