This galaxy exhibits an overall elliptical morphology, appearing elongated or cigar-shaped. The central region presents a concentrated, luminous bulge, transitioning smoothly outward to a less defined, diffuse halo. There is no clear indication of spiral arm structure or significant dust lanes. The galaxy appears relatively smooth in texture with an absence of distinct knots of star formation regions or bright point sources. The color profile suggests a redder hue in the central bulge, possibly indicative of an older stellar population, while the outer regions display a slightly bluer tint, hinting at the presence of younger stars, albeit not prominently. There appears to be no prominent features or major disruptions indicating a recent or ongoing major merger event. There is a suggestion of a very minor disturbance in the evenness of the halo, however it is not a major characteristic.
