The galaxy presents as a slightly elongated, somewhat smooth structure. There's a central concentration of light that transitions into a more diffuse, extended halo. The color profile suggests a relatively evolved stellar population, with a dominant reddish hue near the core, indicating older stars. Faint blue tinges are seen at the periphery, which could indicate some on-going star formation, however, the redness across most of the galaxy suggests that this is dominated by older stellar populations. There is no obvious sign of strong spiral arm structures or a prominent disk, although the slight elongation could indicate a faint disk oriented edge-on. There is no evidence of significant morphological disturbance or ongoing major merger activity.
